This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.40 10:08:44.89 +67:44:59.2
142.53908 42.65830 galactic UMa Second-epoch detections are separated by 1.3" and 2.3 pix
The object was found in VSX 3" Gaia DR3 1067110433150626432
Type: ROT
# Max. Min./Amp. JD0 Period
14.000 G 14.030 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:08:44.89 +67:44:59.2: 14.28 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:08:44.89 +67:44:59.2: 14.34 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.31 +/- 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!
TCP 2026 06 12.3136* 10 08 44.89 +67 44 59.2 13.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1067110433150626432,2461203.8136,13.40,0.05,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
Gaia DR3 1067110433150626432 20260612.3136 13.40CV 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 06 12.3136 2461203.8136 13.36 09:35:48.74 +70:33:06.3
141.67701 38.66305 galactic UMa Second-epoch detections are separated by 1.3" and 1.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:35:48.74 +70:33:06.3 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.030 (K)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:35:48.74 +70:33:06.3: 14.30 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:35:48.74 +70:33:06.3: 14.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.33 +/- 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!
TCP 2026 06 12.3136* 09 35 48.74 +70 33 06.3 13.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.36,0.05,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 20260612.3136 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.24 09:37:39.31 +71:20:50.0
140.70851 38.37806 galactic UMa Second-epoch detections are separated by 1.2" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:37:39.31 +71:20:50.0 (user input) | T | P | (position from user input) J-Ks=0.521+/-0.033 (K)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:37:39.31 +71:20:50.0: 14.17 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:37:39.31 +71:20:50.0: 14.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 09 37 39.31 +71 20 50.0 13.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.24,0.05,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 20260612.3136 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.40 09:50:01.01 +71:18:59.9
140.04059 39.21965 galactic UMa Second-epoch detections are separated by 3.0" and 1.3 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 | 09:50:01.01 +71:18:59.9 (user input) | T | P | (position from user input) J-Ks=0.623+/-0.033 (K)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:50:01.01 +71:18:59.9: 14.36 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:50:01.01 +71:18:59.9: 14.41 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.39 +/- 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!
TCP 2026 06 12.3136* 09 50 01.01 +71 18 59.9 13.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.40,0.05,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
target 20260612.3136 13.40CV 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 06 12.3136 2461203.8136 13.09 10:05:54.13 +70:18:55.6
140.05679 40.86389 galactic UMa Second-epoch detections are separated by 0.5" and 2.1 pix
The object was found in VSX 1" TSVSC1 TN-N213111103-25-82-2
Type: EW
# Max. Min./Amp. JD0 Period
14.315 g Y 0.769 g 2458526.92750 0.255076400000
The object was not found in astcheck.
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:05:54.13 +70:18:55.6: 14.32 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:05:54.13 +70:18:55.6: 14.40 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.35 +/- 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!
TCP 2026 06 12.3136* 10 05 54.13 +70 18 55.6 13.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TSVSC1 TN-N213111103-25-82-2,2461203.8136,13.09,0.05,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
TSVSC1 TN-N213111103-25-82-2 20260612.3136 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.22 10:06:02.50 +69:51:13.6
140.52385 41.16234 galactic UMa Second-epoch detections are separated by 1.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:06:02.50 +69:51:13.6 (user input) | T | P | (position from user input) J-Ks=0.479+/-0.030 (K)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:06:02.50 +69:51:13.6: 14.18 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:06:02.50 +69:51:13.6: 14.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 10 06 02.50 +69 51 13.6 13.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.22,0.05,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 20260612.3136 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.36 09:48:02.00 +70:17:11.5
141.25890 39.66974 galactic UMa Second-epoch detections are separated by 2.2" and 2.3 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 | 09:48:02.00 +70:17:11.5 (user input) | T | P | (position from user input) J-Ks=0.702+/-0.029 (K)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:48:02.00 +70:17:11.5: 14.32 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:48:02.00 +70:17:11.5: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 09 48 02.00 +70 17 11.5 13.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.36,0.05,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 20260612.3136 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.02 09:00:02.39 +72:57:33.5
140.58153 35.08243 galactic UMa Second-epoch detections are separated by 1.7" and 1.6 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 | 09:00:02.39 +72:57:33.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:00:02.39 +72:57:33.5: 13.99 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:00:02.39 +72:57:33.5: 14.10 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 09 00 02.39 +72 57 33.5 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.02,0.05,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 20260612.3136 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.17 09:40:54.50 +71:07:59.2
140.76193 38.71348 galactic UMa Second-epoch detections are separated by 1.7" and 1.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:40:54.50 +71:07:59.2 (user input) | T | P | (position from user input) J-Ks=0.807+/-0.033 (K)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:40:54.50 +71:07:59.2: 14.17 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:40:54.50 +71:07:59.2: 14.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 09 40 54.50 +71 07 59.2 13.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.17,0.05,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 20260612.3136 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.54 10:13:24.89 +67:31:41.6
142.39835 43.14354 galactic UMa Second-epoch detections are separated by 1.0" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:13:24.89 +67:31:41.6 (user input) | T | P | (position from user input) J-Ks=0.386+/-0.034 (G)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:13:24.89 +67:31:41.6: 14.57 +/- 0.08 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:13:24.89 +67:31:41.6: 14.64 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.60 +/- 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!
TCP 2026 06 12.3136* 10 13 24.89 +67 31 41.6 13.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260612.3136 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.52 10:15:17.17 +68:29:11.8
141.23911 42.66584 galactic UMa Second-epoch detections are separated by 1.2" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:15:17.17 +68:29:11.8 (user input) | T | P | (position from user input) J-Ks=0.287+/-0.037 (F)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:15:17.17 +68:29:11.8: 14.44 +/- 0.07 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:15:17.17 +68:29:11.8: 14.65 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.53 +/- 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!
TCP 2026 06 12.3136* 10 15 17.17 +68 29 11.8 13.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260612.3136 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.15 10:02:30.07 +68:32:15.8
142.16946 41.71822 galactic UMa Second-epoch detections are separated by 0.4" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:02:30.07 +68:32:15.8 (user input) | T | P | (position from user input) J-Ks=0.328+/-0.035 (G)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:02:30.07 +68:32:15.8: 14.16 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:02:30.07 +68:32:15.8: 14.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 10 02 30.07 +68 32 15.8 13.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.15,0.05,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 20260612.3136 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.53 10:07:32.48 +69:46:08.9
140.50364 41.31620 galactic UMa Second-epoch detections are separated by 1.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:07:32.48 +69:46:08.9 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.031 (G)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:07:32.48 +69:46:08.9: 14.50 +/- 0.08 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:07:32.48 +69:46:08.9: 14.59 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.54 +/- 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!
TCP 2026 06 12.3136* 10 07 32.48 +69 46 08.9 13.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260612.3136 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 12.66 08:50:31.27 +67:26:25.5
147.30524 36.20155 galactic UMa Second-epoch detections are separated by 1.9" and 1.4 pix
The object was found in VSX 2" OY UMa
Type: EA
# Max. Min./Amp. JD0 Period
13.200 R1 14.200 R1 2451567.76000 1.528030000000
The object was not found in astcheck.
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:50:31.27 +67:26:25.5: 13.80 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:50:31.27 +67:26:25.5: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 08 50 31.27 +67 26 25.5 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
OY UMa,2461203.8136,12.66,0.05,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
OY UMa 20260612.3136 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.24 09:26:48.58 +70:30:34.4
142.19586 38.03148 galactic UMa Second-epoch detections are separated by 1.1" and 1.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:26:48.58 +70:30:34.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:26:48.58 +70:30:34.4: 14.53 +/- 0.07 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:26:48.58 +70:30:34.4: 14.66 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.59 +/- 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!
TCP 2026 06 12.3136* 09 26 48.58 +70 30 34.4 13.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.24,0.05,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 20260612.3136 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.27 09:41:33.37 +70:52:33.8
141.00348 38.89629 galactic UMa Second-epoch detections are separated by 1.1" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:41:33.37 +70:52:33.8 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.032 (G)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:41:33.37 +70:52:33.8: 14.24 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:41:33.37 +70:52:33.8: 14.27 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 09 41 33.37 +70 52 33.8 13.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.27,0.05,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 20260612.3136 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.46 09:52:20.40 +68:59:13.7
142.39288 40.70814 galactic UMa Second-epoch detections are separated by 1.4" and 2.2 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 | 09:52:20.40 +68:59:13.7 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.034 (G)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:52:20.40 +68:59:13.7: 14.41 +/- 0.07 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:52:20.40 +68:59:13.7: 14.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.39 +/- 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!
TCP 2026 06 12.3136* 09 52 20.40 +68 59 13.7 13.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.46,0.05,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 20260612.3136 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.20 10:02:56.71 +68:11:01.1
142.51787 41.96250 galactic UMa Second-epoch detections are separated by 4.3" and 2.3 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 | 10:02:56.71 +68:11:01.1 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.037 (G)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:02:56.71 +68:11:01.1: 14.18 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:02:56.71 +68:11:01.1: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 10 02 56.71 +68 11 01.1 13.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.20,0.05,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 20260612.3136 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 12.96 08:43:14.73 +72:26:11.2
141.70991 34.09814 galactic UMa Second-epoch detections are separated by 1.2" and 1.3 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 | 08:43:14.73 +72:26:11.2 (user input) | T | P | (position from user input) J-Ks=0.588+/-0.034 (K)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:43:14.73 +72:26:11.2: 13.97 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:43:14.73 +72:26:11.2: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 08 43 14.73 +72 26 11.2 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,12.96,0.05,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 20260612.3136 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.65 09:51:29.40 +68:51:04.3
142.59795 40.72093 galactic UMa Second-epoch detections are separated by 4.2" and 1.3 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 | 09:51:29.40 +68:51:04.3 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.033 (G)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:51:29.40 +68:51:04.3: 14.92 +/- 0.11 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:51:29.40 +68:51:04.3: 14.74 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.81 +/- 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!
TCP 2026 06 12.3136* 09 51 29.40 +68 51 04.3 13.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.65,0.05,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 20260612.3136 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.13 10:02:05.54 +69:45:23.6
140.90403 40.95391 galactic UMa Second-epoch detections are separated by 2.1" and 1.6 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 | 10:02:05.54 +69:45:23.6 (user input) | T | P | (position from user input) SpType: M4.5 2004AJ....128..463R LP 37- 57
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:02:05.54 +69:45:23.6: 14.13 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:02:05.54 +69:45:23.6: 14.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 10 02 05.54 +69 45 23.6 13.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.13,0.05,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 20260612.3136 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.20 09:53:23.47 +68:48:30.9
142.51730 40.88692 galactic UMa Second-epoch detections are separated by 2.1" and 1.6 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 | 09:53:23.47 +68:48:30.9 (user input) | T | P | (position from user input) J-Ks=0.832+/-0.030 (M)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:53:23.47 +68:48:30.9: 14.10 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:53:23.47 +68:48:30.9: 14.16 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 09 53 23.47 +68 48 30.9 13.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.20,0.05,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 20260612.3136 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.04 08:56:48.79 +72:51:10.5
140.81229 34.90410 galactic UMa Second-epoch detections are separated by 1.7" and 1.1 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 | target | 08:56:48.79 +72:51:10.5 (user input) | T | P | (position from user input) J-Ks=0.509+/-0.034 (K)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:56:48.79 +72:51:10.5: 13.95 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:56:48.79 +72:51:10.5: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 08 56 48.79 +72 51 10.5 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.04,0.05,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 20260612.3136 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 13.15 09:09:21.04 +70:30:52.5
142.99476 36.72137 galactic UMa Second-epoch detections are separated by 1.1" and 1.6 pix
The object was found in VSX 1" Gaia DR3 1118733741025632640
Type: ROT
# Max. Min./Amp. JD0 Period
13.770 G 13.800 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:09:21.04 +70:30:52.5: 14.11 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:09:21.04 +70:30:52.5: 14.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 09 09 21.04 +70 30 52.5 13.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1118733741025632640,2461203.8136,13.15,0.05,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
Gaia DR3 1118733741025632640 20260612.3136 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3136 2461203.8136 12.70 08:54:39.04 +72:31:28.5
141.25670 34.87583 galactic UMa Second-epoch detections are separated by 1.7" and 1.4 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 | 08:54:39.04 +72:31:28.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:54:39.04 +72:31:28.5: 13.69 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:54:39.04 +72:31:28.5: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 12.3136* 08 54 39.04 +72 31 28.5 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,12.70,0.05,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 20260612.3136 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 06 12.3136 2461203.8136 13.35 09:38:48.02 +69:39:06.0
142.50301 39.34330 galactic UMa Second-epoch detections are separated by 1.7" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:38:48.02 +69:39:06.0 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.033 (K)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:38:48.02 +69:39:06.0: 14.52 +/- 0.07 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:38:48.02 +69:39:06.0: 14.54 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.53 +/- 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!
TCP 2026 06 12.3136* 09 38 48.02 +69 39 06.0 13.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461203.8136,13.35,0.05,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 20260612.3136 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79736027 11.02.2026 07:08:01.927 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
First image: 2461082.79736027 11.02.2026 07:08:01.927 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Last image: 2461203.81388568 12.06.2026 07:31:49.723 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6190
Objects passed selection criteria: 6176
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 5013
Average stars matched: 4805.5 (95.8608 %)
Memory usage VmPeak: 112624 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jun 12 04:29:45 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79736027 11.02.2026 07:08:01.927 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
First image: 2461082.79736027 11.02.2026 07:08:01.927 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Last image: 2461203.81388568 12.06.2026 07:31:49.723 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 100
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 22 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 37627
Objects passed selection criteria: 37517
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 29176.2
Average stars matched: 28010 (96.0027 %)
Memory usage VmPeak: 142404 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jun 12 04:32:11 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
SExtractor catalog cache: saved UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.cat to cache
SExtractor catalog cache: saved UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.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: 2461203.81338907
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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits exists and is non-empty
Saving wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits to local_wcs_cache/
'wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits' -> 'local_wcs_cache/wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits'
wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits exists and is non-empty
Saving wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits to local_wcs_cache/
'wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits' -> 'local_wcs_cache/wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits'
wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits exists and is non-empty
Saving wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits to local_wcs_cache/
'wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits' -> 'local_wcs_cache/wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits'
wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits exists and is non-empty
Saving wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits to local_wcs_cache/
'wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits' -> 'local_wcs_cache/wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits (1st reference image)
verification OK: wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:36:20.400 +69:59:16.84 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-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits (1st new image)
verification OK: wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
Image size: 937.6'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:36:04.608 +70:00:27.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:36:20.400 +69:59:16.84
Second-epoch image center 09:36:04.608 +70:00:27.39
Angular distance between the image centers 0.0298 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits (2nd new image)
verification OK: wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
Image size: 937.6'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:36:06.074 +70:00:35.15 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:36:20.400 +69:59:16.84
Second-epoch image center 09:36:06.074 +70:00:35.15
Angular distance between the image centers 0.0298 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:36:04.608 +70:00:27.39
Second-epoch second image center 09:36:06.074 +70:00:35.15
Angular distance between the image centers 0.00300 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits &> /tmp/tmp.5w69kQ0PEz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits &> /tmp/tmp.UFZAPe6Vna
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits &> /tmp/tmp.nxVkuX9sDX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits &> /tmp/tmp.1MnW19MNFJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits and wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits and wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
Found non-empty wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits and wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
The reference image (wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits) and catalog (wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat) found
'wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat' -> 'wcsmag.cat'
Read 8779 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 117.0365 to 171.9949 deg, Dec +62.9088 to +75.4797 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 117.0365 to 171.9949 deg, Dec 62.9088 to 75.4797 deg
Loaded 9303 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): 5118 out of 5414 total matches.
Matched with Tycho-2 5414 out of 8779 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.863700
a=0.000000 b=1.000000 c=22.863700
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.35
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.35
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8779 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 117.0365 to 171.9949 deg, Dec +62.9088 to +75.4797 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 117.0365 to 171.9949 deg, Dec 62.9088 to 75.4797 deg
Loaded 9303 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): 5118 out of 5414 total matches.
Matched with Tycho-2 5414 out of 8779 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits:
Forced-photometry filter: calibrated wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits -> calib.txt_param_ref_wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits (aperture=6.0)
Read 8894 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 117.0365 to 171.9944 deg, Dec +62.9087 to +75.4796 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 117.0365 to 171.9944 deg, Dec 62.9087 to 75.4796 deg
Loaded 9303 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): 5136 out of 5418 total matches.
Matched with Tycho-2 5418 out of 8894 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits:
Forced-photometry filter: calibrated wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits -> calib.txt_param_ref_wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
2.1 pix UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
2.8 pix fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
2.8 pix fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
2.1 pix wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
2.1 pix wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Limiting magnitude estimates:
15.4 mag. UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
15.4 mag. UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
13.7 mag. fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
13.7 mag. fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5w69kQ0PEz (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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits' -> 'wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WCS_IMAGE_NAME=wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WCS-calibrated image found: wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Checking if the catalog wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits alredy exist and is non-empty...
Catalog wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WCS catalog name: wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=680, passed=8779
Got 8779 stars (including 8092 good ones) from the SExtractor catalog wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
util/solve_plate_with_UCAC5 got 8779 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 8707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 8708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 8708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits N_match=968 sigma_overall_arcsec=0.393 sigma_q1_arcsec=0.524 sigma_q2_arcsec=0.370 sigma_q3_arcsec=0.416 sigma_q4_arcsec=0.332 n_q1=198 n_q2=294 n_q3=213 n_q4=263 worst_quadrant_to_overall_ratio=1.331
The image catalog is written to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits -region wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.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.UFZAPe6Vna (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-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.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-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.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-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits' -> 'wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WCS_IMAGE_NAME=wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WCS-calibrated image found: wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Checking if the catalog wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits alredy exist and is non-empty...
Catalog wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WCS catalog name: wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=664, passed=8894
Got 8894 stars (including 8220 good ones) from the SExtractor catalog wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat
util/solve_plate_with_UCAC5 got 8894 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 8779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 8779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 8779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits N_match=970 sigma_overall_arcsec=0.395 sigma_q1_arcsec=0.509 sigma_q2_arcsec=0.376 sigma_q3_arcsec=0.417 sigma_q4_arcsec=0.318 n_q1=198 n_q2=284 n_q3=224 n_q4=264 worst_quadrant_to_overall_ratio=1.288
The image catalog is written to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits -region wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.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.nxVkuX9sDX (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
WCS_IMAGE_NAME=wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
WCS-calibrated image found: wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
Checking if the catalog wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
WCS catalog name: wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=273, passed=4773
Got 4773 stars (including 4500 good ones) from the SExtractor catalog wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat
util/solve_plate_with_UCAC5 got 4773 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 4725 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 4724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 4724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits N_match=965 sigma_overall_arcsec=0.623 sigma_q1_arcsec=0.484 sigma_q2_arcsec=0.834 sigma_q3_arcsec=0.500 sigma_q4_arcsec=0.780 n_q1=233 n_q2=267 n_q3=259 n_q4=206 worst_quadrant_to_overall_ratio=1.340
The image catalog is written to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits -region wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.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.1MnW19MNFJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
WCS_IMAGE_NAME=wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
WCS-calibrated image found: wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
Checking if the catalog wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
WCS catalog name: wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat
SExtractor catalog parsing summary: zero_flux=16, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=425, passed=5087
Got 5087 stars (including 4659 good ones) from the SExtractor catalog wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat
util/solve_plate_with_UCAC5 got 5087 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5046 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5046 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5046 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits N_match=965 sigma_overall_arcsec=0.644 sigma_q1_arcsec=0.448 sigma_q2_arcsec=1.074 sigma_q3_arcsec=0.551 sigma_q4_arcsec=0.788 n_q1=241 n_q2=268 n_q3=258 n_q4=198 worst_quadrant_to_overall_ratio=1.667
The image catalog is written to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits -region wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits sigma_overall=0.393 worst_q_ratio=1.331
ref2=UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits sigma_overall=0.395 worst_q_ratio=1.288
new1=fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits sigma_overall=0.623 worst_q_ratio=1.340
new2=fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits sigma_overall=0.644 worst_q_ratio=1.667
reference average sigma_overall=0.394 worst_q_ratio=1.3095
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292_astrometric_residuals.png (968 matched stars from wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293_astrometric_residuals.png (970 matched stars from wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114_astrometric_residuals.png (965 matched stars from wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.57 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115_astrometric_residuals.png (965 matched stars from wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.59 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits'
Saving fully-calibrated image wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits'
Preparing the HTML report for the field UMa-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:56:28.23 +65:19:55.6: 11.26 +/- 0.00 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:55:06.75 +65:14:32.8: 10.52 +/- 0.00 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:56:28.23 +65:19:55.6: 11.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.00
Forced photometry filter REJECTED candidate at 08:56:28.23 +65:19:55.6: ref_mag=11.25 +/- 0.00 new_mean_mag=11.3432 delta=-0.09 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:55:06.75 +65:14:32.8: 10.53 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.53 +/- 0.00
Forced photometry filter REJECTED candidate at 08:55:06.75 +65:14:32.8: ref_mag=10.53 +/- 0.00 new_mean_mag=10.8474 delta=-0.32 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20509_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 20509_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20590_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 20590_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04529_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 04529_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
**** FOUND 09:37:34.49 +69:58:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01377_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 01377_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:55:39.52 +71:52:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04047_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 04047_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:44:37.62 +68:46:33.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field UMa-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
SExtractor catalog cache: saved UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.cat to cache
SExtractor catalog cache: saved UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Creating symlink local_wcs_cache/wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits exists and is non-empty
wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits exists and is non-empty
wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits exists and is non-empty
wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits (1st reference image)
verification OK: wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:36:20.400 +69:59:16.84 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-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits (1st new image)
verification OK: wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
Image size: 937.6'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:36:04.608 +70:00:27.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:36:20.400 +69:59:16.84
Second-epoch image center 09:36:04.608 +70:00:27.39
Angular distance between the image centers 0.0298 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits (2nd new image)
verification OK: wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
Image size: 937.6'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:36:06.074 +70:00:35.15 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:36:20.400 +69:59:16.84
Second-epoch image center 09:36:06.074 +70:00:35.15
Angular distance between the image centers 0.0298 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:36:04.608 +70:00:27.39
Second-epoch second image center 09:36:06.074 +70:00:35.15
Angular distance between the image centers 0.00300 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits &> /tmp/tmp.Zs7nPgyv1X
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits &> /tmp/tmp.6yVd2WZZrB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits &> /tmp/tmp.Srv3sg7Z9e
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits &> /tmp/tmp.GOeK9izNri
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits and wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits and wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
Found non-empty wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits and wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
The reference image (wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits) and catalog (wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat) found
'wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat' -> 'wcsmag.cat'
Read 51532 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 116.7773 to 172.6837 deg, Dec +62.8130 to +75.4851 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 116.7773 to 172.6837 deg, Dec 62.8130 to 75.4851 deg
Loaded 9545 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): 4868 out of 5492 total matches.
Matched with Tycho-2 5492 out of 51532 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.743500
a=0.000000 b=1.000000 c=22.743500
From vast_summary.log: estimated ref. image limiting mag.: -7.19
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.55
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.55
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 51532 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 116.7773 to 172.6837 deg, Dec +62.8130 to +75.4851 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 116.7773 to 172.6837 deg, Dec 62.8130 to 75.4851 deg
Loaded 9545 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): 4868 out of 5492 total matches.
Matched with Tycho-2 5492 out of 51532 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits:
Forced-photometry filter: calibrated wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits -> calib.txt_param_ref_wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits (aperture=4.6)
Read 51887 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 116.7032 to 172.5255 deg, Dec +62.8134 to +75.4919 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 116.7032 to 172.5255 deg, Dec 62.8134 to 75.4919 deg
Loaded 9544 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): 4857 out of 5495 total matches.
Matched with Tycho-2 5495 out of 51887 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits:
Forced-photometry filter: calibrated wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits -> calib.txt_param_ref_wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 68 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
1.9 pix UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
2.6 pix fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
2.6 pix fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
1.9 pix wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
1.9 pix wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Limiting magnitude estimates:
15.6 mag. UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
15.6 mag. UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
13.9 mag. fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
14.0 mag. fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Zs7nPgyv1X (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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.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-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits' -> 'wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WCS_IMAGE_NAME=wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WCS-calibrated image found: wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Checking if the catalog wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits alredy exist and is non-empty...
Catalog wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WCS catalog name: wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=2624, passed=51522
Got 51522 stars (including 48803 good ones) from the SExtractor catalog wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
util/solve_plate_with_UCAC5 got 51522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 51013 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
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 51011 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 51012 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits N_match=968 sigma_overall_arcsec=0.412 sigma_q1_arcsec=0.527 sigma_q2_arcsec=0.358 sigma_q3_arcsec=0.456 sigma_q4_arcsec=0.319 n_q1=207 n_q2=283 n_q3=214 n_q4=264 worst_quadrant_to_overall_ratio=1.277
The image catalog is written to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits -region wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.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.6yVd2WZZrB (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-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.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-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.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-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits' -> 'wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WCS_IMAGE_NAME=wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WCS-calibrated image found: wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Checking if the catalog wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits alredy exist and is non-empty...
Catalog wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WCS catalog name: wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=2687, passed=51868
Got 51868 stars (including 49084 good ones) from the SExtractor catalog wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat
util/solve_plate_with_UCAC5 got 51868 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 51377 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
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 51376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 51376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits N_match=971 sigma_overall_arcsec=0.392 sigma_q1_arcsec=0.459 sigma_q2_arcsec=0.361 sigma_q3_arcsec=0.416 sigma_q4_arcsec=0.329 n_q1=214 n_q2=276 n_q3=217 n_q4=264 worst_quadrant_to_overall_ratio=1.170
The image catalog is written to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits -region wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.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.Srv3sg7Z9e (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
WCS_IMAGE_NAME=wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
WCS-calibrated image found: wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
Checking if the catalog wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
WCS catalog name: wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1523, passed=22791
Got 22791 stars (including 21241 good ones) from the SExtractor catalog wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat
util/solve_plate_with_UCAC5 got 22791 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 22501 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 22503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 22503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits N_match=964 sigma_overall_arcsec=0.611 sigma_q1_arcsec=0.492 sigma_q2_arcsec=0.849 sigma_q3_arcsec=0.483 sigma_q4_arcsec=0.836 n_q1=256 n_q2=238 n_q3=275 n_q4=195 worst_quadrant_to_overall_ratio=1.390
The image catalog is written to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits -region wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.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.GOeK9izNri (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
WCS_IMAGE_NAME=wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
WCS-calibrated image found: wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
Checking if the catalog wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
WCS catalog name: wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat
SExtractor catalog parsing summary: zero_flux=26, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1607, passed=23676
Got 23676 stars (including 22050 good ones) from the SExtractor catalog wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat
util/solve_plate_with_UCAC5 got 23676 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 23435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 23436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 23436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits N_match=964 sigma_overall_arcsec=0.624 sigma_q1_arcsec=0.487 sigma_q2_arcsec=1.050 sigma_q3_arcsec=0.526 sigma_q4_arcsec=0.773 n_q1=267 n_q2=236 n_q3=269 n_q4=192 worst_quadrant_to_overall_ratio=1.682
The image catalog is written to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits -region wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.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-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-06_20.00sec_5.00C_LIGHT_0114.fits
Saving fully-calibrated image wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_UMa-01-Q2b1x1_023441_TTUQ2b1x1_3517537_R684tju4/wcs_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115.fits
Preparing the HTML report for the field UMa-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:55:06.74 +65:14:32.7: 10.52 +/- 0.00 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:56:28.22 +65:19:55.5: 11.28 +/- 0.00 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:55:33.16 +65:37:38.3: 10.06 +/- 0.00 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:58:41.84 +65:34:24.0: 10.15 +/- 0.00 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:56:30.46 +65:30:14.5: 12.48 +/- 0.01 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:54:56.38 +65:40:34.0: 11.97 +/- 0.01 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:54:06.35 +65:49:09.6: 11.75 +/- 0.01 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:54:56.46 +65:34:04.3: 12.07 +/- 0.01 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:55:06.74 +65:14:32.7: 10.54 +/- 0.00 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:56:28.22 +65:19:55.5: 11.25 +/- 0.00 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:58:41.84 +65:34:24.0: 10.14 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.53 +/- 0.00
Forced photometry filter REJECTED candidate at 08:55:06.74 +65:14:32.7: ref_mag=10.53 +/- 0.00 new_mean_mag=10.7251 delta=-0.19 (need > 0.90)
Forced photometry reference-image weighted average: 10.14 +/- 0.00
Forced photometry reference-image weighted average: 11.27 +/- 0.00
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:55:33.16 +65:37:38.3: 10.04 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 08:58:41.84 +65:34:24.0: ref_mag=10.14 +/- 0.00 new_mean_mag=10.2079 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:56:28.22 +65:19:55.5: ref_mag=11.27 +/- 0.00 new_mean_mag=11.2228 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 10.05 +/- 0.00
Forced photometry filter REJECTED candidate at 08:55:33.16 +65:37:38.3: ref_mag=10.05 +/- 0.00 new_mean_mag=10.2124 delta=-0.16 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:53:37.97 +65:52:08.3: 12.69 +/- 0.02 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:54:06.35 +65:49:09.6: 11.75 +/- 0.01 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:54:56.38 +65:40:34.0: 12.03 +/- 0.01 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:56:30.46 +65:30:14.5: 12.49 +/- 0.01 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:54:56.46 +65:34:04.3: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.00
Forced photometry filter REJECTED candidate at 08:54:06.35 +65:49:09.6: ref_mag=11.75 +/- 0.00 new_mean_mag=11.5459 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 08:54:56.38 +65:40:34.0: ref_mag=12.00 +/- 0.01 new_mean_mag=11.7660 delta=0.23 (need > 0.90)
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter REJECTED candidate at 08:56:30.46 +65:30:14.5: ref_mag=12.49 +/- 0.01 new_mean_mag=12.2065 delta=0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:54:56.46 +65:34:04.3: ref_mag=12.09 +/- 0.01 new_mean_mag=11.8617 delta=0.22 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:55:06.20 +65:20:04.3: 12.59 +/- 0.01 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:53:37.97 +65:52:08.3: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter REJECTED candidate at 08:53:37.97 +65:52:08.3: ref_mag=12.69 +/- 0.01 new_mean_mag=12.3268 delta=0.36 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:58:04.59 +65:23:28.7: 12.84 +/- 0.02 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:55:06.20 +65:20:04.3: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter REJECTED candidate at 08:55:06.20 +65:20:04.3: ref_mag=12.58 +/- 0.01 new_mean_mag=12.2901 delta=0.29 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:57:03.45 +65:27:45.5: 13.02 +/- 0.02 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:59:49.37 +65:28:37.5: 13.22 +/- 0.02 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:54:57.57 +65:16:41.3: 13.11 +/- 0.02 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:55:25.87 +65:15:24.7: 13.30 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:58:04.59 +65:23:28.7: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter REJECTED candidate at 08:58:04.59 +65:23:28.7: ref_mag=12.82 +/- 0.01 new_mean_mag=12.4574 delta=0.37 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:57:03.45 +65:27:45.5: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter REJECTED candidate at 08:57:03.45 +65:27:45.5: ref_mag=13.04 +/- 0.02 new_mean_mag=12.6224 delta=0.41 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:54:57.57 +65:16:41.3: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter REJECTED candidate at 08:54:57.57 +65:16:41.3: ref_mag=13.08 +/- 0.02 new_mean_mag=12.7661 delta=0.31 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:56:10.16 +65:34:29.5: 13.63 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:59:49.37 +65:28:37.5: 13.20 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:54:00.76 +65:44:33.5: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter REJECTED candidate at 08:59:49.37 +65:28:37.5: ref_mag=13.21 +/- 0.02 new_mean_mag=12.6779 delta=0.53 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:55:25.87 +65:15:24.7: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter REJECTED candidate at 08:55:25.87 +65:15:24.7: ref_mag=13.29 +/- 0.02 new_mean_mag=12.9259 delta=0.37 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:57:13.92 +65:25:11.1: 13.50 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:56:28.37 +65:24:59.0: 13.39 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:56:10.16 +65:34:29.5: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Forced photometry filter REJECTED candidate at 08:56:10.16 +65:34:29.5: ref_mag=13.61 +/- 0.03 new_mean_mag=13.0284 delta=0.58 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:54:00.76 +65:44:33.5: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter REJECTED candidate at 08:54:00.76 +65:44:33.5: ref_mag=13.32 +/- 0.02 new_mean_mag=12.8237 delta=0.50 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:57:13.92 +65:25:11.1: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry filter REJECTED candidate at 08:57:13.92 +65:25:11.1: ref_mag=13.49 +/- 0.02 new_mean_mag=12.9307 delta=0.56 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:56:28.37 +65:24:59.0: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter REJECTED candidate at 08:56:28.37 +65:24:59.0: ref_mag=13.40 +/- 0.02 new_mean_mag=13.0062 delta=0.39 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:08:44.89 +67:44:59.2: 14.28 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:35:48.74 +70:33:06.3: 14.30 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:50:01.01 +71:18:59.9: 14.36 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:37:39.31 +71:20:50.0: 14.17 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:05:54.13 +70:18:55.6: 14.32 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:08:44.89 +67:44:59.2: 14.34 +/- 0.07 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:06:02.50 +69:51:13.6: 14.18 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:35:48.74 +70:33:06.3: 14.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.05
Forced photometry filter KEPT candidate at 10:08:44.89 +67:44:59.2: ref_mag=14.31 +/- 0.05 new_mean_mag=13.4067 delta=0.90 (need > 0.90)
Forced photometry reference-image weighted average: 14.33 +/- 0.05
Forced photometry filter KEPT candidate at 09:35:48.74 +70:33:06.3: ref_mag=14.33 +/- 0.05 new_mean_mag=13.3459 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:37:39.31 +71:20:50.0: 14.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.04
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:50:01.01 +71:18:59.9: 14.41 +/- 0.07 detection
Forced photometry filter KEPT candidate at 09:37:39.31 +71:20:50.0: ref_mag=14.15 +/- 0.04 new_mean_mag=13.2367 delta=0.91 (need > 0.90)
Forced photometry reference-image weighted average: 14.39 +/- 0.05
Forced photometry filter KEPT candidate at 09:50:01.01 +71:18:59.9: ref_mag=14.39 +/- 0.05 new_mean_mag=13.3621 delta=1.02 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:11:10.61 +69:08:43.4: 14.20 +/- 0.07 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:05:54.13 +70:18:55.6: 14.40 +/- 0.07 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:06:02.50 +69:51:13.6: 14.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.05
Forced photometry reference-image weighted average: 14.15 +/- 0.04
Forced photometry filter KEPT candidate at 10:06:02.50 +69:51:13.6: ref_mag=14.15 +/- 0.04 new_mean_mag=13.2234 delta=0.92 (need > 0.90)
Forced photometry filter KEPT candidate at 10:05:54.13 +70:18:55.6: ref_mag=14.35 +/- 0.05 new_mean_mag=13.1179 delta=1.24 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:48:02.00 +70:17:11.5: 14.32 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:00:02.39 +72:57:33.5: 13.99 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:11:10.61 +69:08:43.4: 14.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.05
Forced photometry filter REJECTED candidate at 10:11:10.61 +69:08:43.4: ref_mag=14.23 +/- 0.05 new_mean_mag=13.5202 delta=0.71 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:48:02.00 +70:17:11.5: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.04
Forced photometry filter KEPT candidate at 09:48:02.00 +70:17:11.5: ref_mag=14.26 +/- 0.04 new_mean_mag=13.3525 delta=0.91 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:00:02.39 +72:57:33.5: 14.10 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.04
Forced photometry filter KEPT candidate at 09:00:02.39 +72:57:33.5: ref_mag=14.04 +/- 0.04 new_mean_mag=13.0096 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:40:54.50 +71:07:59.2: 14.17 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:40:54.50 +71:07:59.2: 14.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.03
Forced photometry filter KEPT candidate at 09:40:54.50 +71:07:59.2: ref_mag=14.11 +/- 0.03 new_mean_mag=13.1794 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:13:24.89 +67:31:41.6: 14.57 +/- 0.08 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:13:24.89 +67:31:41.6: 14.64 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.06
Forced photometry filter KEPT candidate at 10:13:24.89 +67:31:41.6: ref_mag=14.60 +/- 0.06 new_mean_mag=13.5199 delta=1.08 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:15:17.17 +68:29:11.8: 14.44 +/- 0.07 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:02:30.07 +68:32:15.8: 14.16 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:15:17.17 +68:29:11.8: 14.65 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.06
Forced photometry filter KEPT candidate at 10:15:17.17 +68:29:11.8: ref_mag=14.53 +/- 0.06 new_mean_mag=13.5007 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:02:30.07 +68:32:15.8: 14.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.04
Forced photometry filter KEPT candidate at 10:02:30.07 +68:32:15.8: ref_mag=14.18 +/- 0.04 new_mean_mag=13.1574 delta=1.02 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:07:32.48 +69:46:08.9: 14.50 +/- 0.08 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:50:31.27 +67:26:25.5: 13.80 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:07:32.48 +69:46:08.9: 14.59 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.06
Forced photometry filter KEPT candidate at 10:07:32.48 +69:46:08.9: ref_mag=14.54 +/- 0.06 new_mean_mag=13.5262 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:50:31.27 +67:26:25.5: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.03
Forced photometry filter KEPT candidate at 08:50:31.27 +67:26:25.5: ref_mag=13.82 +/- 0.03 new_mean_mag=12.6597 delta=1.16 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:26:48.58 +70:30:34.4: 14.53 +/- 0.07 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:41:33.37 +70:52:33.8: 14.24 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:26:48.58 +70:30:34.4: 14.66 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.06
Forced photometry filter KEPT candidate at 09:26:48.58 +70:30:34.4: ref_mag=14.59 +/- 0.06 new_mean_mag=13.2335 delta=1.36 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:41:33.37 +70:52:33.8: 14.27 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.04
Forced photometry filter KEPT candidate at 09:41:33.37 +70:52:33.8: ref_mag=14.25 +/- 0.04 new_mean_mag=13.2715 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:52:20.40 +68:59:13.7: 14.41 +/- 0.07 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:02:56.71 +68:11:01.1: 14.18 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:52:20.40 +68:59:13.7: 14.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.05
Forced photometry filter KEPT candidate at 09:52:20.40 +68:59:13.7: ref_mag=14.39 +/- 0.05 new_mean_mag=13.4227 delta=0.97 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:02:56.71 +68:11:01.1: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.04
Forced photometry filter KEPT candidate at 10:02:56.71 +68:11:01.1: ref_mag=14.20 +/- 0.04 new_mean_mag=13.1640 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:43:14.73 +72:26:11.2: 13.97 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:43:14.73 +72:26:11.2: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.04
Forced photometry filter KEPT candidate at 08:43:14.73 +72:26:11.2: ref_mag=13.99 +/- 0.04 new_mean_mag=12.9571 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:51:29.40 +68:51:04.3: 14.92 +/- 0.11 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:51:29.40 +68:51:04.3: 14.74 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.07
Forced photometry filter KEPT candidate at 09:51:29.40 +68:51:04.3: ref_mag=14.81 +/- 0.07 new_mean_mag=13.5986 delta=1.22 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:02:05.54 +69:45:23.6: 14.13 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:02:05.54 +69:45:23.6: 14.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Forced photometry filter KEPT candidate at 10:02:05.54 +69:45:23.6: ref_mag=14.10 +/- 0.04 new_mean_mag=13.1265 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:53:23.47 +68:48:30.9: 14.10 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:56:48.79 +72:51:10.5: 13.95 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:53:23.47 +68:48:30.9: 14.16 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.04
Forced photometry filter KEPT candidate at 09:53:23.47 +68:48:30.9: ref_mag=14.12 +/- 0.04 new_mean_mag=13.1955 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:56:48.79 +72:51:10.5: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Forced photometry filter KEPT candidate at 08:56:48.79 +72:51:10.5: ref_mag=13.96 +/- 0.04 new_mean_mag=13.0446 delta=0.92 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:09:21.04 +70:30:52.5: 14.11 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:09:21.04 +70:30:52.5: 14.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.04
Forced photometry filter KEPT candidate at 09:09:21.04 +70:30:52.5: ref_mag=14.12 +/- 0.04 new_mean_mag=13.1391 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:54:39.04 +72:31:28.5: 13.69 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:38:48.02 +69:39:06.0: 14.52 +/- 0.07 detection
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:54:39.04 +72:31:28.5: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Forced photometry filter KEPT candidate at 08:54:39.04 +72:31:28.5: ref_mag=13.69 +/- 0.03 new_mean_mag=12.6846 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-01-Q2b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:38:48.02 +69:39:06.0: 14.54 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.05
Forced photometry filter KEPT candidate at 09:38:48.02 +69:39:06.0: ref_mag=14.53 +/- 0.05 new_mean_mag=13.3487 delta=1.18 (need > 0.90)
Adding exclusion_list_local.txt__out13148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50835.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 53s
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: 16s
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Considering the candidate 64549_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64549_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 64563_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64563_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 64566_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64566_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 64568_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64568_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 64571_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64571_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 64600_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64600_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 64633_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64633_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 64640_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64640_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 64715_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64715_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 64720_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64720_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 64809_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64809_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 64850_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64850_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 64909_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 64909_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65044_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65044_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65066_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65066_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 65070_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65070_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 65075_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65075_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 65097_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65097_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65098_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65098_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65122_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65122_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 65142_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65142_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65191_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65191_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 65243_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65243_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 65253_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65253_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65325_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65325_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65368_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65368_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65373_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65373_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 65446_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65446_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
**** FOUND 09:58:06.19 +72:51:46.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 65455_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65455_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 65496_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65496_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65503_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65503_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65532_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65532_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65541_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65541_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 65594_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65594_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65714_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65714_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 65887_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 65887_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 50835_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 50835_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
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Considering the candidate 24456_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 24456_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
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Considering the candidate 20348_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 20348_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
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Considering the candidate 19627_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 19627_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
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Considering the candidate 23064_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 23064_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
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Considering the candidate 25255_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 25255_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
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Considering the candidate 27990_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 27990_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
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Considering the candidate 24868_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 24868_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
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Considering the candidate 26816_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 26816_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
**** FOUND 09:37:34.48 +69:58:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13148_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 13148_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21246_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 21246_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49329_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 49329_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37033_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 37033_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
**** FOUND 08:54:00.77 +65:57:26.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30702_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 30702_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32024_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 32024_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25470_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 25470_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07628_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 07628_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:55:39.51 +71:52:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44723_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 44723_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23914_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 23914_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
**** FOUND 10:44:37.62 +68:46:33.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25108_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 25108_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22491_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 22491_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30931_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 30931_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46164_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 46164_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15600_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 15600_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31671_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 31671_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26129_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 26129_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31705_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 31705_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13704_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 13704_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20391_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
The candidate 20391_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25577_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 25577_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15356_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 15356_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28694_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
Preparing report for the candidate 28694_fd_UMa-01-Q2b1x1_2026-06-12_02-31-49_20.00sec_5.00C_LIGHT_0115
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 71s
Prepared the HTML report for the field UMa-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:00:02.39 +72:57:33.5
08:56:48.79 +72:51:10.5
08:54:39.04 +72:31:28.5
08:43:14.73 +72:26:11.2
09:50:01.01 +71:18:59.9
09:37:39.31 +71:20:50.0
09:40:54.50 +71:07:59.2
09:41:33.37 +70:52:33.8
10:05:54.13 +70:18:55.6
09:35:48.74 +70:33:06.3
09:48:02.00 +70:17:11.5
09:26:48.58 +70:30:34.4
10:06:02.50 +69:51:13.6
10:07:32.48 +69:46:08.9
09:09:21.04 +70:30:52.5
10:02:05.54 +69:45:23.6
09:38:48.02 +69:39:06.0
10:15:17.17 +68:29:11.8
09:52:20.40 +68:59:13.7
09:51:29.40 +68:51:04.3
09:53:23.47 +68:48:30.9
10:02:30.07 +68:32:15.8
08:50:31.27 +67:26:25.5
10:02:56.71 +68:11:01.1
10:13:24.89 +67:31:41.6
10:08:44.89 +67:44:59.2
########### Completed UMa-01-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
10:08:44.89 +67:44:59.2
09:35:48.74 +70:33:06.3
09:37:39.31 +71:20:50.0
09:50:01.01 +71:18:59.9
10:05:54.13 +70:18:55.6
10:06:02.50 +69:51:13.6
09:48:02.00 +70:17:11.5
09:00:02.39 +72:57:33.5
09:40:54.50 +71:07:59.2
10:13:24.89 +67:31:41.6
10:15:17.17 +68:29:11.8
10:02:30.07 +68:32:15.8
10:07:32.48 +69:46:08.9
08:50:31.27 +67:26:25.5
09:26:48.58 +70:30:34.4
09:41:33.37 +70:52:33.8
09:52:20.40 +68:59:13.7
10:02:56.71 +68:11:01.1
08:43:14.73 +72:26:11.2
09:51:29.40 +68:51:04.3
10:02:05.54 +69:45:23.6
09:53:23.47 +68:48:30.9
08:56:48.79 +72:51:10.5
09:09:21.04 +70:30:52.5
08:54:39.04 +72:31:28.5
09:38:48.02 +69:39:06.0
###################################################################################
10:08:44.89 +67:44:59.2 -- not an asteroid (will add it to exclusion list)
09:35:48.74 +70:33:06.3 -- not an asteroid (will add it to exclusion list)
09:37:39.31 +71:20:50.0 -- not an asteroid (will add it to exclusion list)
09:50:01.01 +71:18:59.9 -- not an asteroid (will add it to exclusion list)
10:05:54.13 +70:18:55.6 -- not an asteroid (will add it to exclusion list)
10:06:02.50 +69:51:13.6 -- not an asteroid (will add it to exclusion list)
09:48:02.00 +70:17:11.5 -- not an asteroid (will add it to exclusion list)
09:00:02.39 +72:57:33.5 -- not an asteroid (will add it to exclusion list)
09:40:54.50 +71:07:59.2 -- not an asteroid (will add it to exclusion list)
10:13:24.89 +67:31:41.6 -- not an asteroid (will add it to exclusion list)
10:15:17.17 +68:29:11.8 -- not an asteroid (will add it to exclusion list)
10:02:30.07 +68:32:15.8 -- not an asteroid (will add it to exclusion list)
10:07:32.48 +69:46:08.9 -- not an asteroid (will add it to exclusion list)
08:50:31.27 +67:26:25.5 -- not an asteroid (will add it to exclusion list)
09:26:48.58 +70:30:34.4 -- not an asteroid (will add it to exclusion list)
09:41:33.37 +70:52:33.8 -- not an asteroid (will add it to exclusion list)
09:52:20.40 +68:59:13.7 -- not an asteroid (will add it to exclusion list)
10:02:56.71 +68:11:01.1 -- not an asteroid (will add it to exclusion list)
08:43:14.73 +72:26:11.2 -- not an asteroid (will add it to exclusion list)
09:51:29.40 +68:51:04.3 -- not an asteroid (will add it to exclusion list)
10:02:05.54 +69:45:23.6 -- not an asteroid (will add it to exclusion list)
09:53:23.47 +68:48:30.9 -- not an asteroid (will add it to exclusion list)
08:56:48.79 +72:51:10.5 -- not an asteroid (will add it to exclusion list)
09:09:21.04 +70:30:52.5 -- not an asteroid (will add it to exclusion list)
08:54:39.04 +72:31:28.5 -- not an asteroid (will add it to exclusion list)
09:38:48.02 +69:39:06.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
08:43:14.73 +72:26:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:50:31.27 +67:26:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:54:39.04 +72:31:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:56:48.79 +72:51:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:00:02.39 +72:57:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:21.04 +70:30:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:26:48.58 +70:30:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:35:48.74 +70:33:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:37:39.31 +71:20:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:38:48.02 +69:39:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:40:54.50 +71:07:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:41:33.37 +70:52:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:02.00 +70:17:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:50:01.01 +71:18:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:51:29.40 +68:51:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:52:20.40 +68:59:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:53:23.47 +68:48:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:02:05.54 +69:45:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:02:30.07 +68:32:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:02:56.71 +68:11:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:05:54.13 +70:18:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:06:02.50 +69:51:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:32.48 +69:46:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:44.89 +67:44:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:13:24.89 +67:31:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:15:17.17 +68:29:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
08:43:14.73 +72:26:11.2 -- not a known variable star
08:50:31.27 +67:26:25.5 -- a known variable star
08:54:39.04 +72:31:28.5 -- not a known variable star
08:56:48.79 +72:51:10.5 -- not a known variable star
09:00:02.39 +72:57:33.5 -- not a known variable star
09:09:21.04 +70:30:52.5 -- a known variable star
09:26:48.58 +70:30:34.4 -- not a known variable star
09:35:48.74 +70:33:06.3 -- not a known variable star
09:37:39.31 +71:20:50.0 -- not a known variable star
09:38:48.02 +69:39:06.0 -- not a known variable star
09:40:54.50 +71:07:59.2 -- not a known variable star
09:41:33.37 +70:52:33.8 -- not a known variable star
09:48:02.00 +70:17:11.5 -- not a known variable star
09:50:01.01 +71:18:59.9 -- not a known variable star
09:51:29.40 +68:51:04.3 -- not a known variable star
09:52:20.40 +68:59:13.7 -- not a known variable star
09:53:23.47 +68:48:30.9 -- not a known variable star
10:02:05.54 +69:45:23.6 -- not a known variable star
10:02:30.07 +68:32:15.8 -- not a known variable star
10:02:56.71 +68:11:01.1 -- not a known variable star
10:05:54.13 +70:18:55.6 -- a known variable star
10:06:02.50 +69:51:13.6 -- not a known variable star
10:07:32.48 +69:46:08.9 -- not a known variable star
10:08:44.89 +67:44:59.2 -- a known variable star
10:13:24.89 +67:31:41.6 -- not a known variable star
10:15:17.17 +68:29:11.8 -- not a known variable star
Found 22 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
26 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
08:43:14.73 +72:26:11.2
08:50:31.27 +67:26:25.5
08:54:39.04 +72:31:28.5
08:56:48.79 +72:51:10.5
09:00:02.39 +72:57:33.5
09:09:21.04 +70:30:52.5
09:26:48.58 +70:30:34.4
09:35:48.74 +70:33:06.3
09:37:39.31 +71:20:50.0
09:38:48.02 +69:39:06.0
09:40:54.50 +71:07:59.2
09:41:33.37 +70:52:33.8
09:48:02.00 +70:17:11.5
09:50:01.01 +71:18:59.9
09:51:29.40 +68:51:04.3
09:52:20.40 +68:59:13.7
09:53:23.47 +68:48:30.9
10:02:05.54 +69:45:23.6
10:02:30.07 +68:32:15.8
10:02:56.71 +68:11:01.1
10:05:54.13 +70:18:55.6
10:06:02.50 +69:51:13.6
10:07:32.48 +69:46:08.9
10:08:44.89 +67:44:59.2
10:13:24.89 +67:31:41.6
10:15:17.17 +68:29:11.8
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461203.81338907 -observatory V36
07:06:23.45 +24:05:29.1 Mercury (0.3mag)
08:03:24.98 +22:29:23.4 Venus (-4.0mag)
03:01:36.47 +16:37:14.6 Mars (1.3mag)
07:51:53.97 +21:22:37.1 Jupiter (-1.8mag)
00:50:30.52 +02:54:48.3 Saturn (0.8mag)
04:01:10.86 +20:28:15.1 Uranus (5.8mag)
00:16:22.11 +00:18:02.6 Neptune (7.8mag)
20:33:06.97 -23:06:07.4 Pluto (14.5mag)
02:31:39.76 +18:57:53.9 Moon (-9.1mag)
-rw-r--r-- 1 apache apache 361 Jun 12 04:29 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461203.81338907:
07:52:01.09 +21:22:14.8 Io (6.0mag)
07:52:03.57 +21:22:08.7 Europa (6.2mag)
07:52:11.05 +21:21:43.0 Ganymede (5.6mag)
07:51:31.26 +21:23:42.2 Callisto (6.7mag)
07:51:56.50 +20:59:17.5 Himalia (15.6mag)
07:51:58.04 +21:22:23.9 Thebe (16.5mag)
07:51:49.07 +21:12:56.8 Elara (17.6mag)
07:54:17.21 +21:32:04.0 Pasiphae (17.7mag)
07:58:18.02 +21:24:38.9 Carme (18.9mag)
00:50:37.26 +02:54:25.0 Titan (8.6mag)
00:50:29.59 +02:55:02.3 Rhea (9.9mag)
00:50:59.18 +02:57:16.3 Iapetus (11.3mag)
00:50:41.14 +02:54:20.6 Hyperion (14.6mag)
00:51:07.69 +02:56:09.0 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 12 04:29 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461203.81338907:
17:27:13.49 -35:32:55.0 JWST
18:24:57.04 +27:12:56.7 Chandra
20:30:43.63 +33:10:10.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 12 04:29 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461203.81338907 -observatory V36
18:40:34.39 -32:56:51.0 13.6mag P/2010 H2 (Vales)
05:57:32.55 -68:01:38.0 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:50:34.84 +32:01:21.4 17.5mag C/2017 K2 (PANSTARRS)
17:13:04.91 +15:32:36.6 17.8mag C/2021 G2 (ATLAS)
21:51:43.96 -46:44:06.1 16.5mag P/2021 N1 (ZTF)
23:11:37.98 +31:44:35.8 17.2mag C/2022 E2 (ATLAS)
05:39:05.16 +26:59:44.9 16.5mag C/2022 N2 (PANSTARRS)
09:32:44.28 +30:56:07.4 16.7mag C/2022 QE78 (ATLAS)
08:52:47.39 +04:07:17.8 17.7mag C/2022 R6 (PANSTARRS)
18:25:31.09 +21:40:00.4 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:17:56.47 -11:01:10.4 17.6mag P/2023 B1 (PANSTARRS)
22:12:50.71 +66:46:19.8 17.8mag C/2023 H5 (Lemmon)
17:36:09.40 -07:05:56.9 13.7mag C/2023 R1 (PANSTARRS)
13:16:44.07 +82:02:43.2 18.0mag C/2023 X2 (Lemmon)
07:16:13.61 +64:27:08.2 17.7mag C/2024 A1 (ATLAS)
06:53:28.61 +28:11:23.2 13.8mag C/2024 E1 (Wierzchos)
15:34:06.48 +13:52:14.1 17.4mag C/2024 G6 (ATLAS)
20:10:08.91 +32:20:59.1 14.0mag C/2024 J3 (ATLAS)
04:22:09.38 -15:35:59.0 16.0mag C/2024 T5 (ATLAS)
06:09:44.67 +33:46:44.6 17.9mag C/2025 J1 (Borisov)
11:33:16.88 +52:30:21.9 17.6mag C/2025 L1 (ATLAS)
06:49:45.28 -11:03:37.6 14.5mag C/2025 R3 (PANSTARRS)
09:27:37.52 +23:16:41.2 17.9mag C/2025 V2 (Rankin)
12:39:41.31 +04:40:00.5 17.2mag C/2025 Y1 (ATLAS)
18:05:46.90 +75:59:09.1 17.8mag C/2026 A2 (Bok)
02:07:41.04 +43:42:04.2 16.1mag C/2026 B2 (Sun-Gao)
11:12:17.68 -02:20:10.5 16.5mag A/2026 E1
20:31:06.20 -08:54:58.4 8.5mag 10P/Tempel
11:03:02.13 -01:02:02.2 16.0mag 29P/Schwassmann-Wachmann
03:18:05.28 +26:11:28.1 17.7mag 47P/Ashbrook-Jackson
09:08:46.05 +22:34:57.3 16.9mag 63P/Wild
00:30:23.05 -06:06:49.2 15.7mag 65P/Gunn
06:56:49.11 +33:48:16.6 17.0mag 76P/West-Kohoutek-Ikemura
03:19:09.45 +17:43:34.6 13.8mag 78P/Gehrels
01:29:35.41 +05:43:36.9 15.6mag 88P/Howell
05:07:54.17 +30:34:39.1 15.3mag 93P/Lovas
02:54:43.43 +28:15:56.4 17.5mag 114P/Wiseman-Skiff
07:00:24.46 +32:52:15.3 15.5mag 123P/West-Hartley
09:57:22.63 +12:52:39.4 16.6mag 124P/Mrkos
04:05:50.22 +19:31:01.6 16.3mag 128P/Shoemaker-Holt
04:41:44.98 +19:15:36.9 17.7mag 131P/Mueller
06:15:39.35 +18:09:03.6 15.2mag 141P/Machholz
06:18:32.02 +17:50:23.1 15.1mag 141P-A/Machholz
05:14:35.82 +16:40:35.0 12.0mag 141P-D/Machholz
03:00:33.07 -24:08:28.7 16.7mag 161P/Hartley-IRAS
03:55:11.53 +25:25:24.4 15.0mag 162P/SidingSpring
19:35:59.86 +02:59:02.5 16.6mag 169P/NEAT
00:29:23.68 +03:15:32.0 17.8mag 220P/McNaught
16:49:06.12 -08:17:54.4 16.5mag 235P/LINEAR
07:43:57.07 +35:18:19.9 17.6mag 240P/NEAT
00:43:11.74 -00:42:03.5 16.3mag 260P/McNaught
04:15:30.99 +33:12:35.0 17.5mag 295P/LINEAR
00:16:48.02 -04:42:47.3 17.7mag 320P/McNaught
15:13:27.56 +07:56:32.1 17.4mag 391P/Kowalski
08:10:27.16 +20:38:13.9 17.9mag 450P/LONEOS
07:06:41.50 +41:24:02.1 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 12 04:29 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
-rw-r--r-- 1 apache apache 5.6K Jun 12 04:29 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
-rw-r--r-- 1 apache apache 189K Jun 12 04:29 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:07:51.250 +24:10:15.37 AT 2026ohe 2026-05-16.81 21.59
13:38:05.560 +19:24:23.06 AT 2026ohd 2026-05-16.80 21.01
14:00:47.770 +18:13:38.00 AT 2026ohc 2026-05-16.80 20.77
14:42:20.560 +46:34:25.14 AT 2026ohb 2026-05-12.86 21.63
15:37:36.080 +28:23:57.03 AT 2026oha 2026-05-12.85 21.38
13:11:47.430 +24:23:17.11 AT 2026ogz 2026-04-23.88 21.65
13:28:46.440 +04:10:17.43 AT 2026ogy 2026-05-22.72 21.45
13:19:13.090 +00:02:42.02 AT 2026ogx 2026-05-22.71 22.28
14:22:32.600 -00:42:16.67 AT 2026ogw 2026-05-22.70 21.87
13:41:54.970 +01:03:14.50 AT 2026ogv 2026-05-22.68 22.32
13:39:12.070 +02:04:49.22 AT 2026ogu 2026-05-21.69 22.02
14:31:27.720 +03:25:02.91 AT 2026ogt 2026-05-17.66 22.05
11:12:25.300 +01:12:09.84 AT 2026ogs 2026-05-17.60 22.13
10:57:06.470 -01:19:33.41 AT 2026ogr 2026-05-17.60 22.09
13:46:33.190 +02:44:41.49 AT 2026ogq 2026-05-11.62 22.84
11:13:33.080 +02:44:16.90 AT 2026ogp 2026-05-11.60 22.76
16:42:30.573 -13:46:07.58 AT 2026ogo 2026-05-24.19 21.5377
00:03:44.957 +08:28:44.28 AT 2026ogn 2026-06-05.44 19.2492
22:46:13.996 +03:59:51.65 AT 2026ogm 2026-06-04.43 18.9981
23:07:50.760 -12:36:34.14 AT 2026ogl 2026-06-05.45 19.2023
-rw-r--r-- 1 apache apache 30K Jun 12 04:29 tns_transients_list.txt
