This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf
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 08 06.1746 2461258.6746 12.40 12:34:46.95 +41:13:51.9
135.51825 75.48757 galactic CVn Second-epoch detections are separated by 3.1" and 9.1 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 | ATO J188.6969+41.2299 | 12:34:46.95 +41:13:51.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K5 (LAMOST DR5)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:46.95 +41:13:51.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:46.95 +41:13:51.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J188.6969+41.2299,2461258.6746,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J188.6969+41.2299 20260806.1746 12.40CV 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 08 06.1746 2461258.6746 12.47 12:35:44.62 +40:03:42.5
136.05477 76.66392 galactic CVn Second-epoch detections are separated by 2.0" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:35:44.62 +40:03:42.5 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.033 (G)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:35:44.62 +40:03:42.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:35:44.62 +40:03:42.5: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.6746,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.1746 12.47CV 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 08 06.1746 2461258.6746 12.70 12:32:19.19 +39:59:39.9
138.84537 76.53736 galactic CVn Second-epoch detections are separated by 4.0" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:32:19.19 +39:59:39.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.458+/-0.036 (G)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:32:19.19 +39:59:39.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:32:19.19 +39:59:39.9: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.6746,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.1746 12.70CV 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 08 06.1746 2461258.6746 12.47 12:21:02.07 +40:56:58.1
145.37056 74.82694 galactic CVn Second-epoch detections are separated by 2.0" and 9.4 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 | 12:21:02.07 +40:56:58.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.615+/-0.028 (K)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:21:02.07 +40:56:58.1: 13.39 +/- 0.03 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:21:02.07 +40:56:58.1: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.6746,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.1746 12.47CV 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 08 06.1746 2461258.6746 12.38 12:18:47.94 +42:11:56.0
144.69110 73.52250 galactic CVn Second-epoch detections are separated by 0.9" and 9.4 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 | 12:18:47.94 +42:11:56.0 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.499+/-0.034 (K)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:18:47.94 +42:11:56.0: 13.38 +/- 0.03 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:18:47.94 +42:11:56.0: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.6746,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.1746 12.38CV 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 08 06.1746 2461258.6746 12.79 12:28:19.49 +40:27:46.1
141.17426 75.83604 galactic CVn Second-epoch detections are separated by 2.1" and 9.6 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 | 12:28:19.49 +40:27:46.1 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.400+/-0.030 (G)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:28:19.49 +40:27:46.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:28:19.49 +40:27:46.1: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.6746,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.1746 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1746 2461258.6746 12.80 12:31:26.75 +41:34:43.0
137.49605 74.97942 galactic CVn Second-epoch detections are separated by 1.1" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:31:26.75 +41:34:43.0 (user input) | T | P | (position from user input) J-Ks=0.420+/-0.039 (G)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:31:26.75 +41:34:43.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:31:26.75 +41:34:43.0: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.6746,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.1746 12.80CV 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 08 06.1746 2461258.6746 12.56 12:34:48.96 +39:23:34.6
137.63893 77.25680 galactic CVn Second-epoch detections are separated by 1.7" and 9.3 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 | 12:34:48.96 +39:23:34.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.453+/-0.035 (G)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:48.96 +39:23:34.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:48.96 +39:23:34.6: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.6746,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.1746 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1746 2461258.6746 12.47 12:34:47.63 +39:10:07.6
137.95996 77.46973 galactic CVn Second-epoch detections are separated by 0.6" and 9.5 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 | 12:34:47.63 +39:10:07.6 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.382+/-0.034 (G)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:47.63 +39:10:07.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:47.63 +39:10:07.6: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461258.6746,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.1746 12.47CV 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 08 06.1746 2461258.6746 12.60 12:29:41.31 +41:28:14.9
138.83163 74.97911 galactic CVn Second-epoch detections are separated by 1.1" and 9.3 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 | ATO J187.4228+41.4729 | 12:29:41.31 +41:28:14.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:29:41.31 +41:28:14.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:29:41.31 +41:28:14.9: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J187.4228+41.4729,2461258.6746,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J187.4228+41.4729 20260806.1746 12.60CV 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 08 06.1746 2461258.6746 12.57 12:26:35.15 +41:07:15.5
141.42110 75.10277 galactic CVn Second-epoch detections are separated by 1.4" and 9.6 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 | 12:26:35.15 +41:07:15.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.297+/-0.032 (F)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:26:35.15 +41:07:15.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:26:35.15 +41:07:15.5: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461258.6746,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.1746 12.57CV 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 08 06.1746 2461258.6746 12.29 12:34:49.88 +40:03:11.4
136.79234 76.62487 galactic CVn Second-epoch detections are separated by 0.7" and 9.3 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 | 12:34:49.88 +40:03:11.4 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.354+/-0.036 (G)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:49.88 +40:03:11.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:49.88 +40:03:11.4: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461258.6746,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260806.1746 12.29CV 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: 2461093.80339146 22.02.2026 07:16:43.022 /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
First image: 2461093.80339146 22.02.2026 07:16:43.022 /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
Last image: 2461258.67498030 06.08.2026 04:11:48.298 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.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: 2 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 3338
Objects passed selection criteria: 3330
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 2642.5
Average stars matched: 2306.75 (87.2942 %)
Memory usage VmPeak: 231268 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 5 23:50:26 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: 2461093.80339146 22.02.2026 07:16:43.022 /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
First image: 2461093.80339146 22.02.2026 07:16:43.022 /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
Last image: 2461258.67498030 06.08.2026 04:11:48.298 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 189
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.17
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 17816
Objects passed selection criteria: 17763
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 14390
Average stars matched: 12692.8 (88.2054 %)
Memory usage VmPeak: 247432 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 5 23:51:19 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
SExtractor catalog cache: saved UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.cat to cache
SExtractor catalog cache: saved UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.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: 2461258.67414311
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits exists and is non-empty
Saving wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits to local_wcs_cache/
'wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits' -> 'local_wcs_cache/wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits'
wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits exists and is non-empty
Saving wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits to local_wcs_cache/
'wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits' -> 'local_wcs_cache/wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits'
wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits exists and is non-empty
Saving wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits to local_wcs_cache/
'wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits' -> 'local_wcs_cache/wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits'
wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits exists and is non-empty
Saving wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits to local_wcs_cache/
'wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits' -> 'local_wcs_cache/wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits (1st reference image)
verification OK: wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
Image size: 941.8'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:00:01.624 +38:00:21.08 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits (1st new image)
verification OK: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
Image size: 938.8'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:00:06.895 +38:02:30.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:00:01.624 +38:00:21.08
Second-epoch image center 12:00:06.895 +38:02:30.34
Angular distance between the image centers 0.0399 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits (2nd new image)
verification OK: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
Image size: 938.8'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:00:03.162 +38:03:07.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:00:01.624 +38:00:21.08
Second-epoch image center 12:00:03.162 +38:03:07.53
Angular distance between the image centers 0.0465 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 12:00:06.895 +38:02:30.34
Second-epoch second image center 12:00:03.162 +38:03:07.53
Angular distance between the image centers 0.01602 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits &> /tmp/tmp.VqcS2nNtwk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits &> /tmp/tmp.FQCvapwB1m
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits &> /tmp/tmp.AmooXPKrHV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits &> /tmp/tmp.EJChKIoVJT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits and wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits and wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat
Found non-empty wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits and wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat
The reference image (wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits) and catalog (wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat) found
'wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat' -> 'wcsmag.cat'
Read 5969 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 169.1627 to 190.3064 deg, Dec +32.0983 to +43.3758 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 169.1627 to 190.3064 deg, Dec 32.0983 to 43.3758 deg
Loaded 4131 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): 2949 out of 3133 total matches.
Matched with Tycho-2 3133 out of 5969 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.919300
a=0.000000 b=1.000000 c=22.919300
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5969 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 169.1627 to 190.3064 deg, Dec +32.0983 to +43.3758 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 169.1627 to 190.3064 deg, Dec 32.0983 to 43.3758 deg
Loaded 4131 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): 2949 out of 3133 total matches.
Matched with Tycho-2 3133 out of 5969 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
Forced-photometry filter: calibrated wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits -> calib.txt_param_ref_wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits (aperture=6.4)
Read 5691 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 169.4142 to 190.6314 deg, Dec +32.4425 to +43.2830 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 169.4142 to 190.6314 deg, Dec 32.4425 to 43.2830 deg
Loaded 3978 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): 2993 out of 3103 total matches.
Matched with Tycho-2 3103 out of 5691 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
Forced-photometry filter: calibrated wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits -> calib.txt_param_ref_wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits (aperture=6.4)
____ 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: 10000)
Median FWHM seeing for isolated stars:
2.2 pix UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
2.4 pix UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
2.3 pix fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
2.3 pix fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
Limiting magnitude estimates:
15.5 mag. UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
15.4 mag. UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
12.2 mag. fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
12.3 mag. fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
All-image limiting magnitude estimate: 12.2 (SNR ) 10.0 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.VqcS2nNtwk (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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits' -> 'wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
WCS_IMAGE_NAME=wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
WCS-calibrated image found: wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
Checking if the catalog wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat corresponding to the image wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits alredy exist and is non-empty...
Catalog wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat corresponding to the image wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
WCS catalog name: wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=429, bad_region=1423, passed=5969
Got 5969 stars (including 4219 good ones) from the SExtractor catalog wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat
util/solve_plate_with_UCAC5 got 5969 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4113 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4109 matched stars entering correct_measured_positions(), 4109 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4109 matched stars entering correct_measured_positions(), 4825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4113 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4109 matched stars entering correct_measured_positions(), 4825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4109 matched stars entering correct_measured_positions(), 4825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4109 stars left (next iteration limit 4519)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits N_match=4109 sigma_overall_arcsec=0.453 sigma_q1_arcsec=0.506 sigma_q2_arcsec=0.470 sigma_q3_arcsec=0.432 sigma_q4_arcsec=0.383 n_q1=1274 n_q2=768 n_q3=1337 n_q4=730 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits -region wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.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.FQCvapwB1m (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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.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-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits' -> 'wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
WCS-calibrated image found: wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
Checking if the catalog wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
WCS catalog name: wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=343, bad_region=1415, passed=5691
Got 5691 stars (including 4016 good ones) from the SExtractor catalog wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat
util/solve_plate_with_UCAC5 got 5691 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 3932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3930 matched stars entering correct_measured_positions(), 3930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3930 matched stars entering correct_measured_positions(), 4551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 3932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3930 matched stars entering correct_measured_positions(), 4551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 3930 matched stars entering correct_measured_positions(), 4551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 3930 stars left (next iteration limit 4323)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits N_match=3930 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.339 sigma_q2_arcsec=0.396 sigma_q3_arcsec=0.411 sigma_q4_arcsec=0.372 n_q1=1207 n_q2=757 n_q3=1256 n_q4=710 worst_quadrant_to_overall_ratio=1.086
The image catalog is written to wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits -region wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.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.AmooXPKrHV (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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
WCS_IMAGE_NAME=wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
WCS-calibrated image found: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
Checking if the catalog wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat corresponding to the image wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat corresponding to the image wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
WCS catalog name: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=60, bad_region=93, passed=1015
Got 1015 stars (including 863 good ones) from the SExtractor catalog wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat
util/solve_plate_with_UCAC5 got 1015 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 613 to 668 (Dec 32.6 to 43.3)
Done reading UCAC5 zone files...
Matched 846 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 846 matched stars entering correct_measured_positions(), 832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 846 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 613 to 668 (Dec 32.6 to 43.3)
Done reading UCAC5 zone files...
Matched 846 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 846 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 846 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 846 stars left (next iteration limit 930)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=846 robust_rms=6.428 arcsec worst_quadrant_rms=12.929 arcsec
SIP_REFIT: SIP order 3 trial: matched=846 robust_rms=0.508 arcsec worst_quadrant_rms=0.662 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=846 robust_rms_before=1.156 arcsec robust_rms_before_corrected=0.404 arcsec robust_rms_after=0.508 arcsec worst_quadrant_rms_before=0.455 worst_quadrant_rms_after=0.662
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.455 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits N_match=846 sigma_overall_arcsec=0.417 sigma_q1_arcsec=0.381 sigma_q2_arcsec=0.462 sigma_q3_arcsec=0.437 sigma_q4_arcsec=0.448 n_q1=380 n_q2=158 n_q3=225 n_q4=83 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits -region wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.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.EJChKIoVJT (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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
WCS-calibrated image found: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
Checking if the catalog wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat corresponding to the image wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat corresponding to the image wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
WCS catalog name: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=53, bad_region=71, passed=956
Got 956 stars (including 832 good ones) from the SExtractor catalog wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat
util/solve_plate_with_UCAC5 got 956 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 613 to 668 (Dec 32.6 to 43.3)
Done reading UCAC5 zone files...
Matched 815 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 815 matched stars entering correct_measured_positions(), 795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 815 matched stars entering correct_measured_positions(), 867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 613 to 668 (Dec 32.6 to 43.3)
Done reading UCAC5 zone files...
Matched 815 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 815 matched stars entering correct_measured_positions(), 865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 815 matched stars entering correct_measured_positions(), 865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 815 stars left (next iteration limit 896)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=815 robust_rms=6.098 arcsec worst_quadrant_rms=13.836 arcsec
SIP_REFIT: SIP order 3 trial: matched=815 robust_rms=0.551 arcsec worst_quadrant_rms=0.612 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=815 robust_rms_before=1.230 arcsec robust_rms_before_corrected=0.409 arcsec robust_rms_after=0.551 arcsec worst_quadrant_rms_before=0.417 worst_quadrant_rms_after=0.612
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.417 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits N_match=815 sigma_overall_arcsec=0.433 sigma_q1_arcsec=0.413 sigma_q2_arcsec=0.439 sigma_q3_arcsec=0.437 sigma_q4_arcsec=0.454 n_q1=362 n_q2=158 n_q3=217 n_q4=78 worst_quadrant_to_overall_ratio=1.049
The image catalog is written to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits -region wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits sigma_overall=0.453 worst_q_ratio=1.117
ref2=UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits sigma_overall=0.379 worst_q_ratio=1.086
new1=fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits sigma_overall=0.417 worst_q_ratio=1.107
new2=fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits sigma_overall=0.433 worst_q_ratio=1.049
reference average sigma_overall=0.416 worst_q_ratio=1.1015
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324_astrometric_residuals.png (4109 matched stars from wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212_astrometric_residuals.png (3930 matched stars from wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118_astrometric_residuals.png (846 matched stars from wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119_astrometric_residuals.png (815 matched stars from wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits'
Saving fully-calibrated image wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits'
Preparing the HTML report for the field UMa-13-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field UMa-13-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
SExtractor catalog cache: saved UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.cat to cache
SExtractor catalog cache: saved UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
Creating symlink local_wcs_cache/wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits exists and is non-empty
wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits exists and is non-empty
wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits exists and is non-empty
wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits (1st reference image)
verification OK: wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
Image size: 941.8'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:00:01.624 +38:00:21.08 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits (1st new image)
verification OK: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
Image size: 938.8'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:00:06.895 +38:02:30.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:00:01.624 +38:00:21.08
Second-epoch image center 12:00:06.895 +38:02:30.34
Angular distance between the image centers 0.0399 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits (2nd new image)
verification OK: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
Image size: 938.8'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:00:03.162 +38:03:07.53 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:00:01.624 +38:00:21.08
Second-epoch image center 12:00:03.162 +38:03:07.53
Angular distance between the image centers 0.0465 deg.
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# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 12:00:06.895 +38:02:30.34
Second-epoch second image center 12:00:03.162 +38:03:07.53
Angular distance between the image centers 0.01602 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits &> /tmp/tmp.a5QsyKmuk8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits &> /tmp/tmp.oxO5XvydFH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits &> /tmp/tmp.px33jJd8kQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits &> /tmp/tmp.FFV9FYnc4w
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits and wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits and wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat
Found non-empty wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits and wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat
The reference image (wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits) and catalog (wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat) found
'wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat' -> 'wcsmag.cat'
Read 29244 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 169.0313 to 190.3771 deg, Dec +32.0559 to +43.3841 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 169.0313 to 190.3771 deg, Dec 32.0559 to 43.3841 deg
Loaded 4193 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): 2855 out of 3143 total matches.
Matched with Tycho-2 3143 out of 29244 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.805500
a=0.000000 b=1.000000 c=22.805500
From vast_summary.log: estimated ref. image limiting mag.: -7.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.64
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.64
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29244 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 169.0313 to 190.3771 deg, Dec +32.0559 to +43.3841 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 169.0313 to 190.3771 deg, Dec 32.0559 to 43.3841 deg
Loaded 4193 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): 2855 out of 3143 total matches.
Matched with Tycho-2 3143 out of 29244 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
Forced-photometry filter: calibrated wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits -> calib.txt_param_ref_wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits (aperture=5.0)
Read 27154 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 169.3706 to 190.6770 deg, Dec +32.4425 to +43.2829 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 169.3706 to 190.6770 deg, Dec 32.4425 to 43.2829 deg
Loaded 3994 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): 2928 out of 3127 total matches.
Matched with Tycho-2 3127 out of 27154 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
Forced-photometry filter: calibrated wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits -> calib.txt_param_ref_wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 74 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
2.2 pix UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
2.2 pix fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
2.2 pix fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
Limiting magnitude estimates:
15.6 mag. UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
15.6 mag. UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
12.7 mag. fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
12.7 mag. fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.a5QsyKmuk8 (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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.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-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits' -> 'wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
WCS_IMAGE_NAME=wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
WCS-calibrated image found: wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
Checking if the catalog wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat corresponding to the image wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits alredy exist and is non-empty...
Catalog wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat corresponding to the image wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits
WCS catalog name: wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1139, bad_region=5784, passed=29234
Got 29234 stars (including 22505 good ones) from the SExtractor catalog wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat
util/solve_plate_with_UCAC5 got 29234 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 4869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 24640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 24640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 24640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4869 stars left (next iteration limit 5355)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits N_match=4869 sigma_overall_arcsec=0.432 sigma_q1_arcsec=0.479 sigma_q2_arcsec=0.440 sigma_q3_arcsec=0.414 sigma_q4_arcsec=0.377 n_q1=1519 n_q2=877 n_q3=1610 n_q4=863 worst_quadrant_to_overall_ratio=1.110
The image catalog is written to wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits -region wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.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.oxO5XvydFH (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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.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-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits' -> 'wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
WCS-calibrated image found: wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
Checking if the catalog wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat corresponding to the image wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits
WCS catalog name: wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=983, bad_region=5273, passed=27135
Got 27135 stars (including 21121 good ones) from the SExtractor catalog wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat
util/solve_plate_with_UCAC5 got 27135 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 4885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 23137 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 23137 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 23137 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4885 stars left (next iteration limit 5373)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits N_match=4885 sigma_overall_arcsec=0.387 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.420 sigma_q3_arcsec=0.417 sigma_q4_arcsec=0.388 n_q1=1503 n_q2=971 n_q3=1488 n_q4=923 worst_quadrant_to_overall_ratio=1.084
The image catalog is written to wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits -region wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.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.px33jJd8kQ (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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
WCS_IMAGE_NAME=wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
WCS-calibrated image found: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
Checking if the catalog wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat corresponding to the image wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat corresponding to the image wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
WCS catalog name: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=349, bad_region=515, passed=7038
Got 7038 stars (including 6184 good ones) from the SExtractor catalog wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat
util/solve_plate_with_UCAC5 got 7038 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.6 to 43.3)
Done reading UCAC5 zone files...
Matched 4810 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4808 matched stars entering correct_measured_positions(), 4808 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4808 matched stars entering correct_measured_positions(), 6705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.6 to 43.3)
Done reading UCAC5 zone files...
Matched 4810 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4808 matched stars entering correct_measured_positions(), 6705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 4808 matched stars entering correct_measured_positions(), 6705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 4808 stars left (next iteration limit 5288)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits N_match=4808 sigma_overall_arcsec=0.681 sigma_q1_arcsec=0.658 sigma_q2_arcsec=0.643 sigma_q3_arcsec=0.739 sigma_q4_arcsec=0.674 n_q1=2101 n_q2=760 n_q3=1353 n_q4=594 worst_quadrant_to_overall_ratio=1.085
The image catalog is written to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits -region wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.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.FFV9FYnc4w (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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
WCS-calibrated image found: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
Checking if the catalog wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat corresponding to the image wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat corresponding to the image wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
WCS catalog name: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=324, bad_region=435, passed=6797
Got 6797 stars (including 6041 good ones) from the SExtractor catalog wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat
util/solve_plate_with_UCAC5 got 6797 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.6 to 43.3)
Done reading UCAC5 zone files...
Matched 4715 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4707 matched stars entering correct_measured_positions(), 4707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4707 matched stars entering correct_measured_positions(), 6507 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.6 to 43.3)
Done reading UCAC5 zone files...
Matched 4714 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4707 matched stars entering correct_measured_positions(), 6507 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 4707 matched stars entering correct_measured_positions(), 6507 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 4707 stars left (next iteration limit 5177)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits N_match=4707 sigma_overall_arcsec=0.679 sigma_q1_arcsec=0.661 sigma_q2_arcsec=0.672 sigma_q3_arcsec=0.694 sigma_q4_arcsec=0.703 n_q1=1987 n_q2=790 n_q3=1335 n_q4=595 worst_quadrant_to_overall_ratio=1.035
The image catalog is written to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits -region wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.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-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-10-35_20.00sec_-0.00C_LIGHT_0118.fits
Saving fully-calibrated image wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.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_2026-08-05_CI_UMa-13-Q2b1x1_232316_TTUQ2b1x1_3001962_V9J5ScHf/wcs_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119.fits
Preparing the HTML report for the field UMa-13-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:25:38.30 +41:36:01.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:18.54 +39:47:55.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:30:56.57 +39:42:47.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:35:12.13 +40:07:30.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:46.95 +41:13:51.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:35:29.90 +40:03:51.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:40.63 +39:24:19.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:32:19.19 +39:59:39.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:35:44.62 +40:03:42.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:18.54 +39:47:55.3: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:18.54 +39:47:55.3: ref_mag=13.29 +/- 0.03 new_mean_mag=12.1634 delta=1.13 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:40.63 +39:24:19.8: 13.08 +/- 0.03 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:30:56.57 +39:42:47.2: 13.53 +/- 0.04 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:35:12.13 +40:07:30.6: 13.16 +/- 0.03 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:35:29.90 +40:03:51.6: 13.40 +/- 0.04 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:25:38.30 +41:36:01.3: 13.15 +/- 0.03 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:46.95 +41:13:51.9: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Forced photometry reference-image weighted average: 13.40 +/- 0.04
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:40.63 +39:24:19.8: ref_mag=13.08 +/- 0.03 new_mean_mag=12.0639 delta=1.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.15 +/- 0.03
Forced photometry filter KEPT candidate at 12:35:12.13 +40:07:30.6: ref_mag=13.16 +/- 0.03 new_mean_mag=12.1884 delta=0.97 (need > 0.90)
Forced photometry filter KEPT candidate at 12:30:56.57 +39:42:47.2: ref_mag=13.53 +/- 0.04 new_mean_mag=12.4734 delta=1.06 (need > 0.90)
Forced photometry filter KEPT candidate at 12:35:29.90 +40:03:51.6: ref_mag=13.40 +/- 0.04 new_mean_mag=12.3249 delta=1.07 (need > 0.90)
Forced photometry filter KEPT candidate at 12:34:46.95 +41:13:51.9: ref_mag=13.36 +/- 0.03 new_mean_mag=12.4003 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 12:25:38.30 +41:36:01.3: ref_mag=13.15 +/- 0.03 new_mean_mag=12.2248 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:32:19.19 +39:59:39.9: 14.00 +/- 0.06 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:21:02.07 +40:56:58.1: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.06
Forced photometry filter KEPT candidate at 12:32:19.19 +39:59:39.9: ref_mag=14.00 +/- 0.06 new_mean_mag=12.6920 delta=1.31 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:35:44.62 +40:03:42.5: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.05
Forced photometry filter KEPT candidate at 12:35:44.62 +40:03:42.5: ref_mag=13.80 +/- 0.05 new_mean_mag=12.4673 delta=1.33 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:21:02.07 +40:56:58.1: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 12:21:02.07 +40:56:58.1: ref_mag=13.40 +/- 0.02 new_mean_mag=12.4705 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:28:19.49 +40:27:46.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:18:47.94 +42:11:56.0: 13.38 +/- 0.03 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:31:26.75 +41:34:43.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:17.31 +39:52:51.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:48.96 +39:23:34.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:31:56.52 +40:05:20.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:31:26.75 +41:34:43.0: 13.97 +/- 0.06 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:31:56.52 +40:05:20.5: 13.82 +/- 0.05 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:48.96 +39:23:34.6: 13.82 +/- 0.05 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:18:47.94 +42:11:56.0: 13.42 +/- 0.03 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:17.31 +39:52:51.4: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.06
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry filter KEPT candidate at 12:31:26.75 +41:34:43.0: ref_mag=13.97 +/- 0.06 new_mean_mag=12.8000 delta=1.17 (need > 0.90)
Forced photometry filter KEPT candidate at 12:34:48.96 +39:23:34.6: ref_mag=13.82 +/- 0.05 new_mean_mag=12.5560 delta=1.27 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:28:19.49 +40:27:46.1: 14.17 +/- 0.07 detection
Forced photometry filter KEPT candidate at 12:18:47.94 +42:11:56.0: ref_mag=13.40 +/- 0.02 new_mean_mag=12.3589 delta=1.04 (need > 0.90)
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry filter KEPT candidate at 12:31:56.52 +40:05:20.5: ref_mag=13.82 +/- 0.05 new_mean_mag=12.5685 delta=1.25 (need > 0.90)
Forced photometry filter KEPT candidate at 12:34:17.31 +39:52:51.4: ref_mag=13.82 +/- 0.05 new_mean_mag=12.5807 delta=1.24 (need > 0.90)
Forced photometry reference-image weighted average: 14.17 +/- 0.07
Forced photometry filter KEPT candidate at 12:28:19.49 +40:27:46.1: ref_mag=14.17 +/- 0.07 new_mean_mag=12.7919 delta=1.38 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:27:39.68 +41:31:28.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:47.63 +39:10:07.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:47.63 +39:10:07.6: 13.70 +/- 0.05 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:27:39.68 +41:31:28.8: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.05
Forced photometry filter KEPT candidate at 12:34:47.63 +39:10:07.6: ref_mag=13.70 +/- 0.05 new_mean_mag=12.4691 delta=1.23 (need > 0.90)
Forced photometry reference-image weighted average: 13.72 +/- 0.05
Forced photometry filter KEPT candidate at 12:27:39.68 +41:31:28.8: ref_mag=13.72 +/- 0.05 new_mean_mag=12.6806 delta=1.04 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:33:40.44 +39:21:33.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:33:40.44 +39:21:33.8: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Forced photometry filter KEPT candidate at 12:33:40.44 +39:21:33.8: ref_mag=13.67 +/- 0.04 new_mean_mag=12.5216 delta=1.15 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:33:45.03 +39:26:46.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:33:45.03 +39:26:46.6: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Forced photometry filter KEPT candidate at 12:33:45.03 +39:26:46.6: ref_mag=13.68 +/- 0.04 new_mean_mag=12.6255 delta=1.05 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:29:41.31 +41:28:14.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:29:41.31 +41:28:14.9: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.05
Forced photometry filter KEPT candidate at 12:29:41.31 +41:28:14.9: ref_mag=13.68 +/- 0.05 new_mean_mag=12.5374 delta=1.14 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:32:37.34 +39:47:56.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:32:37.34 +39:47:56.4: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Forced photometry filter KEPT candidate at 12:32:37.34 +39:47:56.4: ref_mag=13.60 +/- 0.04 new_mean_mag=12.4991 delta=1.10 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:27:24.13 +41:39:05.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:26:35.15 +41:07:15.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:59.62 +40:35:09.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:27:24.13 +41:39:05.6: 13.60 +/- 0.04 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:26:35.15 +41:07:15.5: 13.58 +/- 0.04 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:28:23.10 +40:16:35.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:28:14.21 +42:04:17.0: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Forced photometry filter KEPT candidate at 12:27:24.13 +41:39:05.6: ref_mag=13.60 +/- 0.04 new_mean_mag=12.6274 delta=0.97 (need > 0.90)
Forced photometry filter KEPT candidate at 12:26:35.15 +41:07:15.5: ref_mag=13.58 +/- 0.04 new_mean_mag=12.5685 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:28:12.46 +40:58:21.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:59.62 +40:35:09.3: 13.57 +/- 0.04 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:28:14.21 +42:04:17.0: 13.56 +/- 0.04 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:28:23.10 +40:16:35.6: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.04
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:28:12.46 +40:58:21.6: 13.53 +/- 0.04 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:29:54.66 +41:10:54.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:30:04.90 +41:55:52.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:30:22.68 +39:58:05.2: 99.00 +/- 99.00 bad_region
Forced photometry filter KEPT candidate at 12:28:23.10 +40:16:35.6: ref_mag=13.56 +/- 0.04 new_mean_mag=12.5450 delta=1.01 (need > 0.90)
Forced photometry filter KEPT candidate at 12:28:14.21 +42:04:17.0: ref_mag=13.56 +/- 0.04 new_mean_mag=12.5682 delta=0.99 (need > 0.90)
Forced photometry filter KEPT candidate at 12:34:59.62 +40:35:09.3: ref_mag=13.57 +/- 0.04 new_mean_mag=12.4079 delta=1.16 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:49.88 +40:03:11.4: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Forced photometry filter KEPT candidate at 12:28:12.46 +40:58:21.6: ref_mag=13.53 +/- 0.04 new_mean_mag=12.5374 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:29:54.66 +41:10:54.8: 13.51 +/- 0.04 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:30:22.68 +39:58:05.2: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:30:04.90 +41:55:52.3: 13.51 +/- 0.04 detection
Forced photometry filter KEPT candidate at 12:29:54.66 +41:10:54.8: ref_mag=13.51 +/- 0.04 new_mean_mag=12.5204 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:49.88 +40:03:11.4: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Forced photometry filter KEPT candidate at 12:30:22.68 +39:58:05.2: ref_mag=13.47 +/- 0.04 new_mean_mag=12.5293 delta=0.94 (need > 0.90)
Forced photometry filter KEPT candidate at 12:30:04.90 +41:55:52.3: ref_mag=13.51 +/- 0.04 new_mean_mag=12.4757 delta=1.04 (need > 0.90)
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Forced photometry filter KEPT candidate at 12:34:49.88 +40:03:11.4: ref_mag=13.47 +/- 0.04 new_mean_mag=12.2843 delta=1.19 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:33:20.00 +39:13:49.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:28:46.94 +42:01:23.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:33:09.69 +39:25:36.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:31:50.23 +38:05:38.2: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:33:20.00 +39:13:49.4: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Forced photometry filter KEPT candidate at 12:33:20.00 +39:13:49.4: ref_mag=13.48 +/- 0.04 new_mean_mag=12.4103 delta=1.07 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:27:26.32 +41:50:56.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:32:21.25 +39:19:23.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:28:46.94 +42:01:23.7: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Forced photometry filter KEPT candidate at 12:28:46.94 +42:01:23.7: ref_mag=13.46 +/- 0.04 new_mean_mag=12.4423 delta=1.02 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:33:09.69 +39:25:36.2: 13.48 +/- 0.04 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:31:50.23 +38:05:38.2: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Forced photometry filter KEPT candidate at 12:33:09.69 +39:25:36.2: ref_mag=13.48 +/- 0.04 new_mean_mag=12.4729 delta=1.01 (need > 0.90)
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 12:31:50.23 +38:05:38.2: ref_mag=13.45 +/- 0.03 new_mean_mag=12.4637 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:29:38.01 +42:01:09.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:27:26.32 +41:50:56.7: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.04
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:32:21.25 +39:19:23.4: 13.42 +/- 0.03 detection
Forced photometry filter KEPT candidate at 12:27:26.32 +41:50:56.7: ref_mag=13.41 +/- 0.04 new_mean_mag=12.4446 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter KEPT candidate at 12:32:21.25 +39:19:23.4: ref_mag=13.42 +/- 0.03 new_mean_mag=12.3850 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:29:38.01 +42:01:09.0: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Forced photometry filter KEPT candidate at 12:29:38.01 +42:01:09.0: ref_mag=13.39 +/- 0.04 new_mean_mag=12.3874 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:11.53 +40:34:43.9: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:11.53 +40:34:43.9: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Forced photometry filter KEPT candidate at 12:34:11.53 +40:34:43.9: ref_mag=13.39 +/- 0.04 new_mean_mag=12.3650 delta=1.02 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:29:44.78 +41:03:47.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:31:06.97 +37:27:59.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:30:08.07 +41:09:38.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:35:39.14 +40:33:19.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:35:57.91 +41:04:47.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:31:06.97 +37:27:59.7: 13.36 +/- 0.03 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:29:44.78 +41:03:47.4: 13.35 +/- 0.03 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:30:08.07 +41:09:38.0: 13.36 +/- 0.03 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:33:10.25 +40:21:05.6: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter KEPT candidate at 12:31:06.97 +37:27:59.7: ref_mag=13.36 +/- 0.03 new_mean_mag=12.3414 delta=1.01 (need > 0.90)
Forced photometry filter KEPT candidate at 12:29:44.78 +41:03:47.4: ref_mag=13.35 +/- 0.03 new_mean_mag=12.2645 delta=1.08 (need > 0.90)
Forced photometry filter KEPT candidate at 12:30:08.07 +41:09:38.0: ref_mag=13.36 +/- 0.03 new_mean_mag=12.4406 delta=0.91 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:35:39.14 +40:33:19.4: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Forced photometry filter KEPT candidate at 12:35:39.14 +40:33:19.4: ref_mag=13.34 +/- 0.03 new_mean_mag=12.3677 delta=0.97 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:29:31.50 +41:14:10.7: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:35:57.91 +41:04:47.0: 13.36 +/- 0.04 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:33:10.25 +40:21:05.6: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry reference-image weighted average: 13.36 +/- 0.04
Forced photometry filter KEPT candidate at 12:35:57.91 +41:04:47.0: ref_mag=13.36 +/- 0.04 new_mean_mag=12.4107 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 12:33:10.25 +40:21:05.6: ref_mag=13.35 +/- 0.03 new_mean_mag=12.2889 delta=1.06 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:29:31.50 +41:14:10.7: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter KEPT candidate at 12:29:31.50 +41:14:10.7: ref_mag=13.33 +/- 0.03 new_mean_mag=12.3729 delta=0.96 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:30:54.78 +40:25:37.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:35:11.06 +40:01:45.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:31:26.10 +39:34:33.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:30:54.78 +40:25:37.4: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Forced photometry filter KEPT candidate at 12:30:54.78 +40:25:37.4: ref_mag=13.28 +/- 0.03 new_mean_mag=12.2428 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:31:38.76 +40:00:34.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:35:11.06 +40:01:45.1: 13.25 +/- 0.03 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:31:26.10 +39:34:33.0: 13.23 +/- 0.03 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:32:53.26 +39:34:52.4: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Forced photometry filter KEPT candidate at 12:31:26.10 +39:34:33.0: ref_mag=13.23 +/- 0.03 new_mean_mag=12.2828 delta=0.95 (need > 0.90)
Forced photometry filter KEPT candidate at 12:35:11.06 +40:01:45.1: ref_mag=13.25 +/- 0.03 new_mean_mag=12.2468 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:42.08 +41:33:54.6: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:16.15 +38:37:32.4: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:26.21 +39:11:26.3: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:31:38.76 +40:00:34.0: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Forced photometry filter KEPT candidate at 12:31:38.76 +40:00:34.0: ref_mag=13.21 +/- 0.03 new_mean_mag=12.2510 delta=0.96 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:32:53.26 +39:34:52.4: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Forced photometry filter KEPT candidate at 12:32:53.26 +39:34:52.4: ref_mag=13.18 +/- 0.03 new_mean_mag=12.1764 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:42.08 +41:33:54.6: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:42.08 +41:33:54.6: ref_mag=13.16 +/- 0.03 new_mean_mag=12.0878 delta=1.08 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:16.15 +38:37:32.4: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:16.15 +38:37:32.4: ref_mag=13.15 +/- 0.03 new_mean_mag=12.0896 delta=1.06 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:26.21 +39:11:26.3: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:26.21 +39:11:26.3: ref_mag=13.12 +/- 0.03 new_mean_mag=12.0250 delta=1.10 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:34:24.29 +39:40:10.8: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:35:34.46 +40:01:11.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:32:50.35 +39:48:41.0: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:34:24.29 +39:40:10.8: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry filter KEPT candidate at 12:34:24.29 +39:40:10.8: ref_mag=13.08 +/- 0.03 new_mean_mag=11.9737 delta=1.11 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:35:34.46 +40:01:11.0: 12.82 +/- 0.02 detection
Forced photometry on wcs_UMa-13-Q2b1x1_2026-02-22_01-16-43_20.00sec_-15.00C_LIGHT_0324.fits at 12:33:49.73 +39:19:31.9: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter KEPT candidate at 12:35:34.46 +40:01:11.0: ref_mag=12.82 +/- 0.02 new_mean_mag=11.8286 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:32:50.35 +39:48:41.0: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Forced photometry filter KEPT candidate at 12:32:50.35 +39:48:41.0: ref_mag=12.70 +/- 0.02 new_mean_mag=11.7558 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-13-Q2b1x1_2026-05-11_00-30-09_20.00sec_-5.00C_LIGHT_0212.fits at 12:33:49.73 +39:19:31.9: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Forced photometry filter KEPT candidate at 12:33:49.73 +39:19:31.9: ref_mag=12.68 +/- 0.02 new_mean_mag=11.7239 delta=0.96 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out31155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31934.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out22311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32981.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 36s
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: 11s
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Considering the candidate 31418_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31418_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:32:29.27 +40:55:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31464_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31464_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:29.38 +41:16:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31503_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31503_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:40.63 +39:24:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 1.466 1533530996594231424 188.66971369544 +39.40574404353 12.8895 12.3968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31575_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31575_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:35:12.13 +40:07:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.837 1533694274070808320 188.80031906924 +40.12500812052 13.0731 13.1251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31585_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31585_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:25:38.30 +41:36:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.659 1534912154997311104 186.40961464241 +41.60017956937 12.9797 12.4599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31711_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31711_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:18.54 +39:47:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.831 1533592015193770112 188.57754866854 +39.79866964002 12.9652 12.2106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31808_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
Preparing report for the candidate 31808_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
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Considering the candidate 31816_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31816_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:35:29.90 +40:03:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.064 1533690735017755520 188.87458590448 +40.06435106633 13.2375 12.7969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31971_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31971_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:30.30 +40:51:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32017_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32017_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:30:56.57 +39:42:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 1.857 1533764157483215488 187.73636603658 +39.71321215070 13.3508 12.8057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32383_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
Preparing report for the candidate 32383_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
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Considering the candidate 32657_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
Preparing report for the candidate 32657_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
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Considering the candidate 33154_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 33154_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:35:15.16 +41:33:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25550_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
Preparing report for the candidate 25550_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
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Considering the candidate 22311_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
Preparing report for the candidate 22311_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
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Considering the candidate 32981_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
Preparing report for the candidate 32981_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
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Considering the candidate 32970_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32970_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:35:07.69 +41:50:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32651_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32651_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:35:40.70 +41:08:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32633_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
Preparing report for the candidate 32633_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
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Considering the candidate 32409_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32409_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:17.31 +39:52:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.254 1533595489823130112 188.57216350996 +39.88100852810 13.4952 12.8413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32405_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
Preparing report for the candidate 32405_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
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Considering the candidate 32403_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32403_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:47.01 +40:43:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32378_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32378_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:31:56.52 +40:05:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 1.999 1533798693315658752 187.98596232803 +40.08945592604 13.0492 11.9861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32310_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32310_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:36:05.38 +41:49:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32272_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32272_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:27:39.68 +41:31:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 0.557 1534732109968309504 186.91553674624 +41.52463873554 13.5521 12.8673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32187_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
Preparing report for the candidate 32187_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
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Considering the candidate 32180_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32180_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:33:40.44 +39:21:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.488 1533509998498296448 188.41859850540 +39.35950101666 13.4587 12.9751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32177_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32177_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:33:17.61 +40:46:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32175_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32175_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:33:45.03 +39:26:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 1.510 1533510827427777536 188.43799752051 +39.44658286441 13.4719 12.7846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32160_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
Preparing report for the candidate 32160_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
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Considering the candidate 32141_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32141_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:35:40.72 +41:16:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32118_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32118_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:35:44.63 +40:38:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32066_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32066_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:32:37.34 +39:47:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.226 1533603598721338112 188.15563902476 +39.79904606777 13.5144 12.9934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32055_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32055_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:27:24.13 +41:39:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.032 1534927135843210112 186.85016276224 +41.65160107938 13.3986 12.9276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.032#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32054_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
Preparing report for the candidate 32054_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
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Considering the candidate 32025_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32025_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:59.62 +40:35:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.378 1533909430456920960 188.74854749055 +40.58588248109 13.3522 12.7476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32019_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 32019_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:28:23.10 +40:16:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.655 1533851504233498752 187.09565253371 +40.27661523258 13.3633 12.9637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31999_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31999_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:28:14.21 +42:04:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.603 1535033131340902272 187.05873262660 +42.07166001595 13.0312 12.0568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31997_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31997_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:28:12.46 +40:58:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.732 1534636452456726016 187.05165890071 +40.97272514121 13.3575 12.7117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31996_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31996_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:30:04.90 +41:55:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.747 1534829068854236544 187.52032055085 +41.93138936078 13.3886 12.8871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31974_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31974_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:29:54.66 +41:10:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.427 1534665795673239680 187.47783966268 +41.18179122253 13.3208 12.6792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31951_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31951_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:30:22.68 +39:58:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 0.851 1533782372439908608 187.59480852918 +39.96810782017 13.2105 12.6885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31942_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
Preparing report for the candidate 31942_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
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Considering the candidate 31934_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31934_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:33:20.00 +39:13:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.883 1533506944777368576 188.33359949770 +39.23052152120 13.2266 12.8377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31930_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31930_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:28:46.94 +42:01:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.640 1534844260154295296 187.19571166075 +42.02309982171 13.3091 12.7586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31913_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31913_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:33:09.69 +39:25:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 0.589 1533558205211225344 188.29016418878 +39.42673932488 13.0691 12.2524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31899_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31899_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:31:50.23 +38:05:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.040 1519926498705345664 187.95950041129 +38.09448680646 12.8357 11.8961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31884_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31884_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:27:26.32 +41:50:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 1.195 1534933801632433792 186.85998704203 +41.84931424454 13.2327 12.7138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31855_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31855_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:32:21.25 +39:19:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.444 1533553055546227200 188.08846978310 +39.32327681914 13.3375 12.8980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31849_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31849_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:29:38.01 +42:01:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.661 1534865460112864896 187.40861688745 +42.01912946192 13.2946 12.8827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31842_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31842_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:11.53 +40:34:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.434 1533911320242531328 188.54816191380 +40.57878258676 13.1342 12.4982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31800_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31800_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:29:44.78 +41:03:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.049 1534651948698674048 187.43696188427 +41.06322476121 13.1942 12.6130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31794_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31794_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:31:06.97 +37:27:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.314 1519796515815383808 187.77912772091 +37.46652909532 13.0512 12.3720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31793_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31793_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:30:08.07 +41:09:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.570 1534654147721933056 187.53344439916 +41.16047432436 13.1659 12.5992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31792_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31792_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:35:39.14 +40:33:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.747 1533741175113664384 188.91320557494 +40.55557456852 13.2414 12.7532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31786_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31786_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:35:57.91 +41:04:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.389 1533948707933740288 188.99163193217 +41.07943415091 13.2203 12.6037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31781_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31781_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:33:10.25 +40:21:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.771 1533808760719005952 188.29298740483 +40.35158059961 12.8958 12.0190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31755_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31755_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:29:31.50 +41:14:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.056 1534669815762637696 187.38126336332 +41.23631737497 13.1420 12.6133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31747_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31747_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:32:55.52 +41:43:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31719_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31719_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:32:13.64 +41:02:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31710_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31710_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:30:54.78 +40:25:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.937 1533867825109236992 187.72838185976 +40.42681526328 13.1212 12.5743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31683_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31683_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:35:11.06 +40:01:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.329 1533690425780109184 188.79619925948 +40.02917282504 13.0599 12.3927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31670_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31670_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:14.35 +41:38:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31669_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31669_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:31:26.10 +39:34:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.786 1533571815963344768 187.85887549203 +39.57602899551 13.0901 12.6709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31657_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31657_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:32:37.53 +40:44:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31645_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31645_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:31:38.76 +40:00:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.852 1533774641498799360 187.91172127394 +40.00927922779 13.0939 12.5690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31608_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31608_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:32:53.26 +39:34:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.532 1533563054230073856 188.22173425285 +39.58117702702 12.9478 12.4684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31582_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31582_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:42.08 +41:33:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.494 1534395247093097088 188.67520097583 +41.56526184604 13.0131 12.5296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31569_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31569_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:16.15 +38:37:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.757 1521461829254724096 188.56755882765 +38.62564176296 12.9056 12.3542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31539_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31539_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:26.21 +39:11:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.449 1533492818629116160 188.60936908778 +39.19064480857 12.8496 12.3253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31494_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31494_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:34:24.29 +39:40:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.851 1533590095344196224 188.60143268464 +39.66982802673 12.8425 12.3393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31252_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31252_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:35:34.46 +40:01:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 1.292 1533689807304818944 188.89383577666 +40.02002463296 12.5966 11.9666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31171_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31171_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
**** FOUND 12:32:50.35 +39:48:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 0.671 1533603839239522048 188.20992774315 +39.81154323428 12.5685 12.1055 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31155_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119
The candidate 31155_fd_UMa-13-Q2b1x1_2026-08-05_23-11-48_20.00sec_-0.00C_LIGHT_0119 did not pass the final checks
