This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0
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 14.2245 2461205.7245 14.79 11:19:45.11 +50:15:36.4
153.84190 61.00673 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 | 11:19:45.11 +50:15:36.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 11:19:45.11 +50:15:36.4: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 11:19:45.11 +50:15:36.4: 15.89 +/- 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 14.2246* 11 19 45.11 +50 15 36.4 14.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.7245,14.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.2245 14.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.2245 2461205.7245 14.69 10:19:56.26 +48:31:34.3
166.43259 53.79498 galactic UMa Second-epoch detections are separated by 7.4" 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 | 10:19:56.26 +48:31:34.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 10:19:56.26 +48:31:34.3: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 10:19:56.26 +48:31:34.3: 16.02 +/- 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 14.2246* 10 19 56.26 +48 31 34.3 14.7 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,2461205.7245,14.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.2245 14.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.2245 2461205.7245 14.88 11:12:23.86 +42:21:57.5
169.41807 64.74162 galactic UMa Second-epoch detections are separated by 7.1" 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 | 11:12:23.86 +42:21:57.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 11:12:23.86 +42:21:57.5: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 11:12:23.86 +42:21:57.5: 15.96 +/- 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 14.2246* 11 12 23.86 +42 21 57.5 14.9 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,2461205.7245,14.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.2245 14.88CV 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 14.2245 2461205.7245 14.81 10:16:24.65 +44:16:57.5
173.63149 54.60917 galactic UMa Second-epoch detections are separated by 8.2" and 0.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:16:24.65 +44:16:57.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 10:16:24.65 +44:16:57.5: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 10:16:24.65 +44:16:57.5: 16.03 +/- 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 14.2246* 10 16 24.65 +44 16 57.5 14.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461205.7245,14.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260614.2245 14.81CV 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: 2461093.78748612 22.02.2026 06:53:48.801 /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
First image: 2461093.78748612 22.02.2026 06:53:48.801 /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
Last image: 2461205.72474505 14.06.2026 05:23:27.972 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
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): 6279
Objects passed selection criteria: 6275
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 5658
Average stars matched: 5519.5 (97.5521 %)
Memory usage VmPeak: 112328 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 14 00:29:38 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: 2461093.78748612 22.02.2026 06:53:48.801 /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
First image: 2461093.78748612 22.02.2026 06:53:48.801 /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
Last image: 2461205.72474505 14.06.2026 05:23:27.972 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 132
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
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: 14 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): 30079
Objects passed selection criteria: 30000
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 28054
Average stars matched: 27213.5 (97.004 %)
Memory usage VmPeak: 133656 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 14 00:31:15 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/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
SExtractor catalog cache: saved UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.cat to cache
SExtractor catalog cache: saved UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.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-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.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: 2461205.72434396
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits exists and is non-empty
Saving wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits to local_wcs_cache/
'wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits' -> 'local_wcs_cache/wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits'
wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits exists and is non-empty
Saving wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits to local_wcs_cache/
'wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits' -> 'local_wcs_cache/wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits'
wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits exists and is non-empty
Saving wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits to local_wcs_cache/
'wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits' -> 'local_wcs_cache/wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits'
wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits exists and is non-empty
Saving wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits to local_wcs_cache/
'wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits' -> 'local_wcs_cache/wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits (1st reference image)
verification OK: wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.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: 10:48:01.354 +46:00:05.88 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-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits (1st new image)
verification OK: wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
Image size: 941.5'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:48:13.034 +46:00:48.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:48:01.354 +46:00:05.88
Second-epoch image center 10:48:13.034 +46:00:48.13
Angular distance between the image centers 0.0358 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits (2nd new image)
verification OK: wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
Image size: 941.5'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:48:13.749 +46:00:52.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:48:01.354 +46:00:05.88
Second-epoch image center 10:48:13.749 +46:00:52.46
Angular distance between the image centers 0.0381 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:48:13.034 +46:00:48.13
Second-epoch second image center 10:48:13.749 +46:00:52.46
Angular distance between the image centers 0.00239 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-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits &> /tmp/tmp.HacHn4XBEr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits &> /tmp/tmp.f8pz1d9qIT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits &> /tmp/tmp.CaV1C6dqL5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits &> /tmp/tmp.J0fmEncXFh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.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-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits and wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits and wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat
Found non-empty wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits and wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat
The reference image (wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits) and catalog (wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat) found
'wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat' -> 'wcsmag.cat'
Read 6977 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.2907 to 173.9078 deg, Dec +39.8246 to +51.3881 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 149.2907 to 173.9078 deg, Dec 39.8246 to 51.3881 deg
Loaded 4560 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): 3127 out of 3305 total matches.
Matched with Tycho-2 3305 out of 6977 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.930900
a=0.000000 b=1.000000 c=22.930900
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6977 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.2907 to 173.9078 deg, Dec +39.8246 to +51.3881 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 149.2907 to 173.9078 deg, Dec 39.8246 to 51.3881 deg
Loaded 4560 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): 3127 out of 3305 total matches.
Matched with Tycho-2 3305 out of 6977 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits:
Forced-photometry filter: calibrated wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits -> calib.txt_param_ref_wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits (aperture=6.5)
Read 6367 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.7479 to 174.3135 deg, Dec +40.3419 to +51.2583 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 149.7479 to 174.3135 deg, Dec 40.3419 to 51.2583 deg
Loaded 4269 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): 3196 out of 3285 total matches.
Matched with Tycho-2 3285 out of 6367 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits:
Forced-photometry filter: calibrated wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits -> calib.txt_param_ref_wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits (aperture=6.6)
____ 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:
2.2 pix UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
2.4 pix UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
2.4 pix fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
2.4 pix fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
2.2 pix wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
2.4 pix wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
Limiting magnitude estimates:
15.5 mag. UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
15.3 mag. UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
14.8 mag. fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
14.8 mag. fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 12.0 (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.HacHn4XBEr (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.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-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits' -> 'wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
WCS-calibrated image found: wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
Checking if the catalog wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
WCS catalog name: wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=476, passed=6977
Got 6977 stars (including 6493 good ones) from the SExtractor catalog wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 6977 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 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 6892 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 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 6890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 6890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits N_match=955 sigma_overall_arcsec=0.384 sigma_q1_arcsec=0.477 sigma_q2_arcsec=0.373 sigma_q3_arcsec=0.386 sigma_q4_arcsec=0.308 n_q1=223 n_q2=254 n_q3=246 n_q4=232 worst_quadrant_to_overall_ratio=1.244
The image catalog is written to wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits -region wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.f8pz1d9qIT (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-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.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_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.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-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.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-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits' -> 'wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
WCS_IMAGE_NAME=wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
WCS-calibrated image found: wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
Checking if the catalog wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat corresponding to the image wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits alredy exist and is non-empty...
Catalog wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat corresponding to the image wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
WCS catalog name: wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=355, passed=6367
Got 6367 stars (including 6003 good ones) from the SExtractor catalog wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat
util/solve_plate_with_UCAC5 got 6367 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6283 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6285 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6285 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits N_match=958 sigma_overall_arcsec=0.471 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.519 sigma_q3_arcsec=0.437 sigma_q4_arcsec=0.552 n_q1=214 n_q2=261 n_q3=243 n_q4=240 worst_quadrant_to_overall_ratio=1.171
The image catalog is written to wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits -region wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.CaV1C6dqL5 (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_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.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_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
WCS_IMAGE_NAME=wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
WCS-calibrated image found: wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
Checking if the catalog wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat corresponding to the image wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat corresponding to the image wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
WCS catalog name: wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=273, passed=4726
Got 4726 stars (including 4451 good ones) from the SExtractor catalog wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat
util/solve_plate_with_UCAC5 got 4726 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 4679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 4680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 4680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits N_match=960 sigma_overall_arcsec=0.289 sigma_q1_arcsec=0.260 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.263 sigma_q4_arcsec=0.298 n_q1=231 n_q2=231 n_q3=265 n_q4=233 worst_quadrant_to_overall_ratio=1.203
The image catalog is written to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits -region wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.J0fmEncXFh (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_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.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_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
WCS_IMAGE_NAME=wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
WCS-calibrated image found: wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
Checking if the catalog wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat corresponding to the image wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat corresponding to the image wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
WCS catalog name: wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=252, passed=4713
Got 4713 stars (including 4458 good ones) from the SExtractor catalog wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat
util/solve_plate_with_UCAC5 got 4713 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 4668 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 4668 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 4668 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits N_match=958 sigma_overall_arcsec=0.295 sigma_q1_arcsec=0.288 sigma_q2_arcsec=0.341 sigma_q3_arcsec=0.245 sigma_q4_arcsec=0.306 n_q1=229 n_q2=231 n_q3=266 n_q4=232 worst_quadrant_to_overall_ratio=1.157
The image catalog is written to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits -region wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat.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-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits sigma_overall=0.384 worst_q_ratio=1.244
ref2=UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits sigma_overall=0.471 worst_q_ratio=1.171
new1=fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits sigma_overall=0.289 worst_q_ratio=1.203
new2=fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits sigma_overall=0.295 worst_q_ratio=1.157
reference average sigma_overall=0.4275 worst_q_ratio=1.2075
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300_astrometric_residuals.png (955 matched stars from wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183_astrometric_residuals.png (958 matched stars from wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126_astrometric_residuals.png (960 matched stars from wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127_astrometric_residuals.png (958 matched stars from wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits'
Saving fully-calibrated image wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits'
Preparing the HTML report for the field UMa-10-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field UMa-10-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
SExtractor catalog cache: saved UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.cat to cache
SExtractor catalog cache: saved UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.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-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
Creating symlink local_wcs_cache/wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.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-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits exists and is non-empty
wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits exists and is non-empty
wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits exists and is non-empty
wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits (1st reference image)
verification OK: wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.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: 10:48:01.354 +46:00:05.88 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-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits (1st new image)
verification OK: wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
Image size: 941.5'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:48:13.034 +46:00:48.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:48:01.354 +46:00:05.88
Second-epoch image center 10:48:13.034 +46:00:48.13
Angular distance between the image centers 0.0358 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits (2nd new image)
verification OK: wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
Image size: 941.5'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:48:13.749 +46:00:52.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:48:01.354 +46:00:05.88
Second-epoch image center 10:48:13.749 +46:00:52.46
Angular distance between the image centers 0.0381 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:48:13.034 +46:00:48.13
Second-epoch second image center 10:48:13.749 +46:00:52.46
Angular distance between the image centers 0.00239 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-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits &> /tmp/tmp.9f16NgtizL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits &> /tmp/tmp.JBOiS4wJld
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits &> /tmp/tmp.v9ZZc3iG4f
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits &> /tmp/tmp.DEpgGnVIIY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.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-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits and wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits and wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat
Found non-empty wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits and wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat
The reference image (wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits) and catalog (wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat) found
'wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat' -> 'wcsmag.cat'
Read 34182 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.2627 to 173.9078 deg, Dec +39.8246 to +51.4078 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 149.2627 to 173.9078 deg, Dec 39.8246 to 51.4078 deg
Loaded 4573 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): 2964 out of 3314 total matches.
Matched with Tycho-2 3314 out of 34182 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.821150
a=0.000000 b=1.000000 c=22.821150
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 34182 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.2627 to 173.9078 deg, Dec +39.8246 to +51.4078 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 149.2627 to 173.9078 deg, Dec 39.8246 to 51.4078 deg
Loaded 4573 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): 2964 out of 3314 total matches.
Matched with Tycho-2 3314 out of 34182 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits:
Forced-photometry filter: calibrated wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits -> calib.txt_param_ref_wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits (aperture=5.1)
Read 30481 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.6976 to 174.3134 deg, Dec +40.3159 to +51.2658 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 149.6976 to 174.3134 deg, Dec 40.3159 to 51.2658 deg
Loaded 4298 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): 3062 out of 3297 total matches.
Matched with Tycho-2 3297 out of 30481 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits:
Forced-photometry filter: calibrated wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits -> calib.txt_param_ref_wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits (aperture=5.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 103 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
2.2 pix UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
2.3 pix fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
2.3 pix fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
2.1 pix wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
2.2 pix wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
Limiting magnitude estimates:
15.6 mag. UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
15.5 mag. UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
15.0 mag. fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
15.0 mag. fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.9f16NgtizL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.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-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits' -> 'wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
WCS-calibrated image found: wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
Checking if the catalog wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits
WCS catalog name: wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=1513, passed=34161
Got 34161 stars (including 32578 good ones) from the SExtractor catalog wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 34161 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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 33864 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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 33866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 33866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits N_match=960 sigma_overall_arcsec=0.373 sigma_q1_arcsec=0.442 sigma_q2_arcsec=0.359 sigma_q3_arcsec=0.383 sigma_q4_arcsec=0.308 n_q1=222 n_q2=251 n_q3=249 n_q4=238 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits -region wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JBOiS4wJld (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-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.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_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.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-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.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-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits' -> 'wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
WCS_IMAGE_NAME=wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
WCS-calibrated image found: wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
Checking if the catalog wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat corresponding to the image wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits alredy exist and is non-empty...
Catalog wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat corresponding to the image wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits
WCS catalog name: wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=1294, passed=30460
Got 30460 stars (including 29132 good ones) from the SExtractor catalog wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat
util/solve_plate_with_UCAC5 got 30460 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 30161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 30161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 30161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits N_match=959 sigma_overall_arcsec=0.473 sigma_q1_arcsec=0.340 sigma_q2_arcsec=0.510 sigma_q3_arcsec=0.451 sigma_q4_arcsec=0.528 n_q1=223 n_q2=263 n_q3=238 n_q4=235 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits -region wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.v9ZZc3iG4f (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_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.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_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
WCS_IMAGE_NAME=wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
WCS-calibrated image found: wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
Checking if the catalog wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat corresponding to the image wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat corresponding to the image wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
WCS catalog name: wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=710, passed=24251
Got 24251 stars (including 23507 good ones) from the SExtractor catalog wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat
util/solve_plate_with_UCAC5 got 24251 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 24043 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 24043 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 24043 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits N_match=960 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.255 sigma_q2_arcsec=0.366 sigma_q3_arcsec=0.250 sigma_q4_arcsec=0.307 n_q1=236 n_q2=232 n_q3=262 n_q4=230 worst_quadrant_to_overall_ratio=1.280
The image catalog is written to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits -region wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DEpgGnVIIY (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_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.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_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
WCS_IMAGE_NAME=wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
WCS-calibrated image found: wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
Checking if the catalog wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat corresponding to the image wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat corresponding to the image wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
WCS catalog name: wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=814, passed=24250
Got 24250 stars (including 23398 good ones) from the SExtractor catalog wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat
util/solve_plate_with_UCAC5 got 24250 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 24056 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 24055 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 24055 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits N_match=960 sigma_overall_arcsec=0.291 sigma_q1_arcsec=0.282 sigma_q2_arcsec=0.345 sigma_q3_arcsec=0.252 sigma_q4_arcsec=0.299 n_q1=236 n_q2=235 n_q3=259 n_q4=230 worst_quadrant_to_overall_ratio=1.186
The image catalog is written to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits -region wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits.wcscat.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-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.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_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-22-53_20.00sec_-0.00C_LIGHTs_0126.fits
Saving fully-calibrated image wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.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_2026-06-14_CI_UMa-10-Q1b1x1_002720_TTUQ1b1x1_852825_r46rMVY0/wcs_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127.fits
Preparing the HTML report for the field UMa-10-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 10:49:49.20 +44:37:30.1: 13.30 +/- 0.02 detection
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 11:14:13.52 +48:18:49.3: 14.17 +/- 0.06 detection
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 10:49:49.20 +44:37:30.1: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter REJECTED candidate at 10:49:49.20 +44:37:30.1: ref_mag=13.31 +/- 0.02 new_mean_mag=13.6646 delta=-0.35 (need > 0.90)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 10:18:55.61 +49:13:28.6: 13.94 +/- 0.05 detection
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 11:29:28.01 +46:04:38.4: 13.97 +/- 0.06 detection
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 11:14:13.52 +48:18:49.3: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.05
Forced photometry filter REJECTED candidate at 11:14:13.52 +48:18:49.3: ref_mag=14.17 +/- 0.05 new_mean_mag=13.8602 delta=0.31 (need > 0.90)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 10:18:55.61 +49:13:28.6: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Forced photometry filter REJECTED candidate at 10:18:55.61 +49:13:28.6: ref_mag=13.96 +/- 0.04 new_mean_mag=14.0267 delta=-0.07 (need > 0.90)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 11:29:28.01 +46:04:38.4: 13.94 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Forced photometry filter REJECTED candidate at 11:29:28.01 +46:04:38.4: ref_mag=13.96 +/- 0.05 new_mean_mag=14.1206 delta=-0.16 (need > 0.90)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 10:46:25.10 +44:07:02.0: 14.08 +/- 0.06 detection
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 11:14:14.39 +43:50:55.4: 14.28 +/- 0.07 detection
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 10:44:16.33 +44:41:00.5: 14.34 +/- 0.06 detection
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 10:46:25.10 +44:07:02.0: 14.29 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.04
Forced photometry filter REJECTED candidate at 10:46:25.10 +44:07:02.0: ref_mag=14.15 +/- 0.04 new_mean_mag=14.1898 delta=-0.04 (need > 0.90)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 11:14:14.39 +43:50:55.4: 14.26 +/- 0.08 detection
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 11:19:14.39 +47:17:43.6: 14.82 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.05
Forced photometry filter REJECTED candidate at 11:14:14.39 +43:50:55.4: ref_mag=14.27 +/- 0.05 new_mean_mag=14.2924 delta=-0.02 (need > 0.90)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 10:44:16.33 +44:41:00.5: 14.24 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.05
Forced photometry filter REJECTED candidate at 10:44:16.33 +44:41:00.5: ref_mag=14.30 +/- 0.05 new_mean_mag=14.2873 delta=0.01 (need > 0.90)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 11:19:14.39 +47:17:43.6: 14.87 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.08
Forced photometry filter REJECTED candidate at 11:19:14.39 +47:17:43.6: ref_mag=14.84 +/- 0.08 new_mean_mag=14.6091 delta=0.23 (need > 0.90)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 11:19:45.11 +50:15:36.4: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 10:19:56.26 +48:31:34.3: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 11:12:23.86 +42:21:57.5: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 10:16:24.65 +44:16:57.5: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 11:19:45.11 +50:15:36.4: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 10:19:56.26 +48:31:34.3: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 11:25:42.94 +48:17:23.4: 15.01 +/- 0.14 detection
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 11:12:23.86 +42:21:57.5: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 10:16:24.65 +44:16:57.5: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-10-Q1b1x1_2026-02-22_00-53-48_20.00sec_-14.90C_LIGHT_0300.fits at 10:02:46.59 +49:44:08.3: 13.25 +/- 0.03 detection
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 11:25:42.94 +48:17:23.4: 14.89 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.10
Forced photometry filter REJECTED candidate at 11:25:42.94 +48:17:23.4: ref_mag=14.96 +/- 0.10 new_mean_mag=14.6901 delta=0.27 (need > 0.90)
Forced photometry on wcs_UMa-10-Q1b1x1_2026-05-11_00-03-55_20.00sec_-4.90C_LIGHT_0183.fits at 10:02:46.59 +49:44:08.3: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter REJECTED candidate at 10:02:46.59 +49:44:08.3: ref_mag=13.33 +/- 0.02 new_mean_mag=13.1439 delta=0.18 (need > 0.90)
Adding exclusion_list_local.txt__out52981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53037.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 52143_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52143_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 10:28:27.77 +49:50:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52193_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52193_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52199_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52199_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 11:09:56.47 +44:28:32.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 52287_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52287_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52291_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52291_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52300_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52300_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 11:32:04.07 +49:15:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52304_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52304_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52310_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52310_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 11:16:46.05 +49:26:50.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52317_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52317_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52328_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52328_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52332_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52332_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52351_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52351_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52355_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52355_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52361_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52361_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52382_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52382_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 11:20:39.52 +45:00:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52450_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52450_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 10:59:42.59 +50:10:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52473_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52473_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52478_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52478_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52505_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52505_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52525_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52525_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52530_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52530_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 10:27:52.75 +42:58:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52532_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52532_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52533_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52533_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52540_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52540_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52547_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52547_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52551_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52551_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52578_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52578_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
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Considering the candidate 52597_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52597_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52598_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52598_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52605_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52605_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52620_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52620_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52625_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52625_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52632_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52632_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52641_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52641_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
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Considering the candidate 52644_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52644_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52645_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52645_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52656_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52656_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52672_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52672_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52696_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52696_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 10:13:55.54 +43:34:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52706_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52706_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 10:05:53.92 +45:37:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52711_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52711_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 10:56:05.59 +43:25:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52714_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52714_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 10:54:31.68 +45:27:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52725_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52725_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52726_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52726_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
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Considering the candidate 52729_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52729_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52737_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52737_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
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Considering the candidate 52752_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52752_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 10:57:24.84 +43:55:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52754_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52754_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52760_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52760_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52778_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52778_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 11:30:25.27 +47:49:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52797_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52797_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 11:02:33.30 +48:09:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52798_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52798_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52802_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52802_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52804_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52804_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52808_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52808_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52809_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52809_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52824_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52824_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
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Considering the candidate 52825_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52825_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52829_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52829_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52833_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52833_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
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Considering the candidate 52840_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52840_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52849_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52849_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
**** FOUND 10:53:11.42 +50:59:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52877_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52877_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
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Considering the candidate 52878_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52878_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52894_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52894_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52914_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52914_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52916_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52916_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
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Considering the candidate 52921_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52921_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52924_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52924_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52930_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52930_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52935_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52935_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52939_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52939_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52942_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52942_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52945_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52945_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52946_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52946_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52959_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52959_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52960_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52960_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52972_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52972_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52975_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52975_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 52981_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
Preparing report for the candidate 52981_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
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Considering the candidate 52989_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 52989_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53000_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53000_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 53003_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53003_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53006_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53006_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53009_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
Preparing report for the candidate 53009_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
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Considering the candidate 53011_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53011_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53019_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53019_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 53026_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53026_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53032_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
Preparing report for the candidate 53032_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
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Considering the candidate 53035_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53035_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53037_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
Preparing report for the candidate 53037_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
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Considering the candidate 53040_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53040_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53052_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53052_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 53059_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53059_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53065_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53065_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53068_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53068_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53074_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53074_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
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Considering the candidate 53075_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53075_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 53100_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53100_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53102_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53102_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53113_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53113_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 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 53122_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 53122_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 50042_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127
The candidate 50042_fd_UMa-10-Q1b1x1_2026-06-14_00-23-27_20.00sec_-0.00C_LIGHTs_0127 did not pass the final checks