This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48
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 20.1884 2461211.6884 10.54 09:30:43.08 +65:32:16.4
147.70449 40.62121 galactic UMa Second-epoch detections are separated by 0.4" and 3.5 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 | Gaia DR3 1067989664496102016 | 09:30:43.27 +65:32:18.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:30:43.08 +65:32:16.4: 11.45 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:30:43.08 +65:32:16.4: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.00
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 20.1884* 09 30 43.08 +65 32 16.4 10.5 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
Gaia DR3 1067989664496102016,2461211.6884,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1067989664496102016 20260620.1884 10.54CV 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 20.1884 2461211.6884 11.25 09:45:16.75 +63:49:01.8
148.80810 42.78991 galactic UMa Second-epoch detections are separated by 2.4" and 3.7 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 | Gaia DR3 1063819938446733696 | 09:45:16.70 +63:49:02.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.244+/-0.027 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:45:16.75 +63:49:01.8: 12.27 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:45:16.75 +63:49:01.8: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
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 20.1884* 09 45 16.75 +63 49 01.8 11.2 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 1063819938446733696,2461211.6884,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1063819938446733696 20260620.1884 11.25CV 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 20.1884 2461211.6884 11.59 09:32:25.64 +65:40:43.3
147.43553 40.71793 galactic UMa Second-epoch detections are separated by 1.9" and 3.5 pix
The object was found in VSX 2" Gaia DR3 1067998009616278784
Type: ROT
# Max. Min./Amp. JD0 Period
12.510 G 12.530 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:32:25.64 +65:40:43.3: 12.79 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:32:25.64 +65:40:43.3: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
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 20.1884* 09 32 25.64 +65 40 43.3 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1067998009616278784,2461211.6884,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1067998009616278784 20260620.1884 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.1884 2461211.6884 10.97 09:44:16.47 +63:54:52.8
148.76239 42.64632 galactic UMa Second-epoch detections are separated by 0.9" and 3.5 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 | Gaia DR3 1063824989328279680 | 09:44:16.48 +63:54:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.294+/-0.026 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:44:16.47 +63:54:52.8: 11.86 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:44:16.47 +63:54:52.8: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
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 20.1884* 09 44 16.47 +63 54 52.8 11.0 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
Gaia DR3 1063824989328279680,2461211.6884,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1063824989328279680 20260620.1884 10.97CV 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 20.1884 2461211.6884 11.35 09:46:13.84 +63:35:04.1
149.01927 42.99318 galactic UMa Second-epoch detections are separated by 0.6" and 3.4 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 | Gaia DR3 1063755303482748416 | 09:46:14.22 +63:35:02.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:46:13.84 +63:35:04.1: 12.37 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:46:13.84 +63:35:04.1: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
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 20.1884* 09 46 13.84 +63 35 04.1 11.3 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
Gaia DR3 1063755303482748416,2461211.6884,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1063755303482748416 20260620.1884 11.35CV 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
Mean magnitude and position on the discovery images:
2026 06 20.1884 2461211.6884 10.86 09:47:33.28 +64:14:46.1
148.13227 42.80146 galactic UMa Second-epoch detections are separated by 2.5" and 3.2 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 | Gaia DR3 1063929541715623296 | 09:47:33.46 +64:14:46.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.692+/-0.029 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:47:33.28 +64:14:46.1: 11.84 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:47:33.28 +64:14:46.1: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
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 20.1884* 09 47 33.28 +64 14 46.1 10.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1063929541715623296,2461211.6884,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1063929541715623296 20260620.1884 10.86CV 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 20.1884 2461211.6884 10.90 09:34:09.52 +64:53:38.6
148.26150 41.22734 galactic UMa Second-epoch detections are separated by 0.7" and 3.3 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 | Gaia DR3 1064898731152009216 | 09:34:09.50 +64:53:38.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.029 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:34:09.52 +64:53:38.6: 11.81 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:34:09.52 +64:53:38.6: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
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 20.1884* 09 34 09.52 +64 53 38.6 10.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1064898731152009216,2461211.6884,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064898731152009216 20260620.1884 10.90CV 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 20.1884 2461211.6884 10.88 09:31:38.67 +65:04:10.9
148.20605 40.91150 galactic UMa Second-epoch detections are separated by 0.6" and 3.5 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 | Gaia DR3 1067917612123892736 | 09:31:38.69 +65:04:10.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.506+/-0.029 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:31:38.67 +65:04:10.9: 11.80 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:31:38.67 +65:04:10.9: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
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 20.1884* 09 31 38.67 +65 04 10.9 10.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1067917612123892736,2461211.6884,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1067917612123892736 20260620.1884 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.1884 2461211.6884 11.38 09:34:06.72 +64:42:35.1
148.48459 41.30397 galactic UMa Second-epoch detections are separated by 2.3" and 3.8 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 | Large-amplitude variable Gaia DR2 1064891962283548160 | 09:34:06.77 +64:42:34.5 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.564+/-0.029 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:34:06.72 +64:42:35.1: 12.35 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:34:06.72 +64:42:35.1: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
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 20.1884* 09 34 06.72 +64 42 35.1 11.4 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
Large-amplitude variable Gaia DR2 1064891962283548160,2461211.6884,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1064891962283548160 20260620.1884 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.1884 2461211.6884 11.34 09:43:48.60 +63:39:24.0
149.10511 42.72198 galactic UMa Second-epoch detections are separated by 2.5" and 3.8 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 | Gaia DR3 1063793893765089280 | 09:43:48.78 +63:39:24.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.220+/-0.028 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:43:48.60 +63:39:24.0: 12.32 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:43:48.60 +63:39:24.0: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
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 20.1884* 09 43 48.60 +63 39 24.0 11.3 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
Gaia DR3 1063793893765089280,2461211.6884,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1063793893765089280 20260620.1884 11.34CV 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 20.1884 2461211.6884 11.04 09:48:01.75 +64:47:03.5
147.46121 42.58024 galactic UMa Second-epoch detections are separated by 1.5" and 3.7 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 | Gaia DR3 1064709374633806080 | 09:48:01.78 +64:47:03.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.416+/-0.034 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:48:01.75 +64:47:03.5: 12.31 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:48:01.75 +64:47:03.5: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
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 20.1884* 09 48 01.75 +64 47 03.5 11.0 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
Gaia DR3 1064709374633806080,2461211.6884,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064709374633806080 20260620.1884 11.04CV 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 20.1884 2461211.6884 9.65 09:46:54.02 +65:14:32.8
147.00361 42.24863 galactic UMa Second-epoch detections are separated by 0.8" and 3.4 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 | Gaia DR3 1064803898274029184 | 09:46:54.11 +65:14:32.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.717+/-0.031 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:46:54.02 +65:14:32.8: 10.56 +/- 0.00 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:46:54.02 +65:14:32.8: 10.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.57 +/- 0.00
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 20.1884* 09 46 54.02 +65 14 32.8 9.7 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
Gaia DR3 1064803898274029184,2461211.6884,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064803898274029184 20260620.1884 9.65CV 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 20.1884 2461211.6884 11.31 09:30:26.20 +65:47:40.2
147.41711 40.48332 galactic UMa Second-epoch detections are separated by 1.8" and 3.7 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 | Gaia DR3 1068013780736178688 | 09:30:26.22 +65:47:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.606+/-0.030 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:30:26.20 +65:47:40.2: 12.26 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:30:26.20 +65:47:40.2: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
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 20.1884* 09 30 26.20 +65 47 40.2 11.3 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
Gaia DR3 1068013780736178688,2461211.6884,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1068013780736178688 20260620.1884 11.31CV 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 20.1884 2461211.6884 11.27 09:43:42.57 +64:29:24.3
148.11479 42.31953 galactic UMa Second-epoch detections are separated by 1.2" and 3.6 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 | Gaia DR3 1064608013405381120 | 09:43:42.63 +64:29:24.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-0.028 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:43:42.57 +64:29:24.3: 12.25 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:43:42.57 +64:29:24.3: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
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 20.1884* 09 43 42.57 +64 29 24.3 11.3 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
Gaia DR3 1064608013405381120,2461211.6884,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064608013405381120 20260620.1884 11.27CV 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 20.1884 2461211.6884 10.97 09:33:49.67 +65:31:05.8
147.54015 40.91889 galactic UMa Second-epoch detections are separated by 0.8" and 3.5 pix
The object was found in VSX 2" ASASSN-V J093349.77+653107.5
Type: L
# Max. Min./Amp. JD0 Period
12.540 V 12.790 V
The object was not found in astcheck.
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:33:49.67 +65:31:05.8: 12.20 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:33:49.67 +65:31:05.8: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
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 20.1884* 09 33 49.67 +65 31 05.8 11.0 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
ASASSN-V J093349.77+653107.5,2461211.6884,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J093349.77+653107.5 20260620.1884 10.97CV 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 20.1884 2461211.6884 10.57 09:42:12.74 +65:15:34.2
147.30659 41.81230 galactic UMa Second-epoch detections are separated by 0.7" and 3.5 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 | Gaia DR3 1064980472969623424 | 09:42:12.85 +65:15:34.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:42:12.74 +65:15:34.2: 11.55 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:42:12.74 +65:15:34.2: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.00
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 20.1884* 09 42 12.74 +65 15 34.2 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1064980472969623424,2461211.6884,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064980472969623424 20260620.1884 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.1884 2461211.6884 11.13 09:48:56.10 +64:42:51.0
147.47825 42.69896 galactic UMa Second-epoch detections are separated by 0.4" and 3.4 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 | Gaia DR3 1064719025424247552 | 09:48:56.08 +64:42:50.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.345+/-0.031 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:48:56.10 +64:42:51.0: 12.19 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:48:56.10 +64:42:51.0: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
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 20.1884* 09 48 56.10 +64 42 51.0 11.1 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
Gaia DR3 1064719025424247552,2461211.6884,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064719025424247552 20260620.1884 11.13CV 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 20.1884 2461211.6884 11.12 09:45:55.68 +63:59:49.2
148.54639 42.76685 galactic UMa Second-epoch detections are separated by 1.4" and 3.2 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 | Gaia DR3 1063828047344987008 | 09:45:55.64 +63:59:48.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.284+/-0.033 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:45:55.68 +63:59:49.2: 12.16 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:45:55.68 +63:59:49.2: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
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 20.1884* 09 45 55.68 +63 59 49.2 11.1 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
Gaia DR3 1063828047344987008,2461211.6884,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1063828047344987008 20260620.1884 11.12CV 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 20.1884 2461211.6884 12.28 07:39:50.17 +58:29:22.1
158.72353 29.09429 galactic Lyn Second-epoch detections are separated by 1.4" and 3.5 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 | ATO J114.9602+58.5011 | 07:39:50.17 +58:29:22.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.581+/-0.033 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:39:50.17 +58:29:22.1: 13.24 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:39:50.17 +58:29:22.1: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J114.9602+58.5011,2461211.6884,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J114.9602+58.5011 20260620.1884 12.28CV 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 20.1884 2461211.6884 11.04 09:45:23.74 +64:12:43.8
148.32746 42.61265 galactic UMa Second-epoch detections are separated by 1.5" and 3.2 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 | Gaia DR3 1064586057532582528 | 09:45:23.79 +64:12:44.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.330+/-0.029 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:45:23.74 +64:12:43.8: 12.15 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:45:23.74 +64:12:43.8: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
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 20.1884* 09 45 23.74 +64 12 43.8 11.0 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
Gaia DR3 1064586057532582528,2461211.6884,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064586057532582528 20260620.1884 11.04CV 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 20.1884 2461211.6884 11.52 09:46:06.21 +64:54:06.2
147.46006 42.34430 galactic UMa Second-epoch detections are separated by 2.2" and 3.7 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 | 09:46:06.21 +64:54:06.2 (user input) | T | P | (position from user input) J-Ks=0.680+/-0.033 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:46:06.21 +64:54:06.2: 12.94 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:46:06.21 +64:54:06.2: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.1884* 09 46 06.21 +64 54 06.2 11.5 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,2461211.6884,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.1884 11.52CV 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 20.1884 2461211.6884 10.51 09:44:07.45 +64:34:21.2
147.98800 42.31931 galactic UMa Second-epoch detections are separated by 0.8" and 3.5 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 | Gaia DR3 1064655670362974208 | 09:44:07.33 +64:34:20.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.433+/-0.026 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:44:07.45 +64:34:21.2: 11.45 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:44:07.45 +64:34:21.2: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.00
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 20.1884* 09 44 07.45 +64 34 21.2 10.5 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
Gaia DR3 1064655670362974208,2461211.6884,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064655670362974208 20260620.1884 10.51CV 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 20.1884 2461211.6884 11.93 07:38:05.92 +57:29:04.4
159.84018 28.76603 galactic Lyn Second-epoch detections are separated by 0.9" and 3.7 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 | ATO J114.5246+57.4845 | 07:38:05.92 +57:29:04.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=1.061+/-0.033 (M)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:38:05.92 +57:29:04.4: 12.96 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:38:05.92 +57:29:04.4: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J114.5246+57.4845,2461211.6884,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J114.5246+57.4845 20260620.1884 11.93CV 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 20.1884 2461211.6884 11.07 09:48:05.93 +64:33:09.2
147.72964 42.70178 galactic UMa Second-epoch detections are separated by 1.4" and 3.2 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 | Gaia DR3 1064690030101137920 | 09:48:06.03 +64:33:09.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.317+/-0.035 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:48:05.93 +64:33:09.2: 12.10 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:48:05.93 +64:33:09.2: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
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 20.1884* 09 48 05.93 +64 33 09.2 11.1 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
Gaia DR3 1064690030101137920,2461211.6884,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064690030101137920 20260620.1884 11.07CV 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 20.1884 2461211.6884 12.26 07:35:05.46 +58:01:16.0
159.18282 28.42587 galactic Lyn Second-epoch detections are separated by 1.2" and 3.5 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 | 07:35:05.46 +58:01:16.0 (user input) | T | P | (position from user input) J-Ks=0.667+/-0.033 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:35:05.46 +58:01:16.0: 13.21 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:35:05.46 +58:01:16.0: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.6884,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.1884 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.1884 2461211.6884 10.38 09:48:44.91 +64:24:40.3
147.84961 42.83263 galactic UMa Second-epoch detections are separated by 0.3" and 3.4 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 | Gaia DR3 1063937517470818048 | 09:48:44.95 +64:24:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1956PMcCO..13a....B AG+64 482 J-Ks=0.457+/-0.031 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:48:44.91 +64:24:40.3: 11.38 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:48:44.91 +64:24:40.3: 11.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.37 +/- 0.00
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 20.1884* 09 48 44.91 +64 24 40.3 10.4 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 1063937517470818048,2461211.6884,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1063937517470818048 20260620.1884 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.1884 2461211.6884 11.04 09:40:55.12 +65:30:23.3
147.10235 41.57590 galactic UMa Second-epoch detections are separated by 2.0" and 3.1 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 | Gaia DR3 1065034349039404544 | 09:40:55.11 +65:30:22.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.221+/-0.032 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:40:55.12 +65:30:23.3: 12.08 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:40:55.12 +65:30:23.3: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
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 20.1884* 09 40 55.12 +65 30 23.3 11.0 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
Gaia DR3 1065034349039404544,2461211.6884,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1065034349039404544 20260620.1884 11.04CV 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 20.1884 2461211.6884 12.24 07:41:17.31 +57:07:53.0
160.29219 29.15826 galactic Lyn Second-epoch detections are separated by 0.6" and 3.6 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 | 07:41:17.31 +57:07:53.0 (user input) | T | P | (position from user input) J-Ks=0.372+/-0.034 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:41:17.31 +57:07:53.0: 13.21 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:41:17.31 +57:07:53.0: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461211.6884,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260620.1884 12.24CV 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 20.1884 2461211.6884 11.43 09:46:11.58 +64:26:22.4
148.00032 42.57847 galactic UMa Second-epoch detections are separated by 1.0" and 3.6 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 | Gaia DR3 1064685391536468096 | 09:46:11.59 +64:26:21.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.417+/-0.030 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:46:11.58 +64:26:22.4: 12.55 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:46:11.58 +64:26:22.4: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
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 20.1884* 09 46 11.58 +64 26 22.4 11.4 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 1064685391536468096,2461211.6884,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064685391536468096 20260620.1884 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.1884 2461211.6884 10.38 09:48:37.76 +64:35:51.8
147.63779 42.72877 galactic UMa Second-epoch detections are separated by 0.5" and 3.4 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 | Gaia DR3 1064691713728316800 | 09:48:37.82 +64:35:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.753+/-0.034 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:48:37.76 +64:35:51.8: 11.33 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:48:37.76 +64:35:51.8: 11.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.00
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 20.1884* 09 48 37.76 +64 35 51.8 10.4 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 1064691713728316800,2461211.6884,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064691713728316800 20260620.1884 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.1884 2461211.6884 11.45 09:46:33.88 +65:11:52.5
147.07943 42.24028 galactic UMa Second-epoch detections are separated by 0.5" and 3.5 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 | Gaia DR3 1064802626963711360 | 09:46:33.95 +65:11:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.595+/-0.032 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:46:33.88 +65:11:52.5: 12.52 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:46:33.88 +65:11:52.5: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
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 20.1884* 09 46 33.88 +65 11 52.5 11.4 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 1064802626963711360,2461211.6884,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064802626963711360 20260620.1884 11.45CV 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 20.1884 2461211.6884 11.10 09:37:43.78 +64:21:46.1
148.66915 41.80646 galactic UMa Second-epoch detections are separated by 1.1" and 3.6 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 | Gaia DR3 1064640689516626048 | 09:37:43.84 +64:21:45.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-0.028 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:37:43.78 +64:21:46.1: 12.04 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:37:43.78 +64:21:46.1: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
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 20.1884* 09 37 43.78 +64 21 46.1 11.1 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
Gaia DR3 1064640689516626048,2461211.6884,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064640689516626048 20260620.1884 11.10CV 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 20.1884 2461211.6884 11.39 09:41:29.85 +63:35:28.3
149.34498 42.52424 galactic UMa Second-epoch detections are separated by 3.0" and 3.0 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 | Gaia DR3 1063790350415430016 | 09:41:30.01 +63:35:27.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.426+/-0.026 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:41:29.85 +63:35:28.3: 12.52 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:41:29.85 +63:35:28.3: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
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 20.1884* 09 41 29.85 +63 35 28.3 11.4 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 1063790350415430016,2461211.6884,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1063790350415430016 20260620.1884 11.39CV 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 20.1884 2461211.6884 10.99 09:46:51.72 +64:24:43.1
147.98525 42.65495 galactic UMa Second-epoch detections are separated by 1.3" and 3.6 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 | Gaia DR3 1064682878979387392 | 09:46:51.79 +64:24:42.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.381+/-0.031 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:46:51.72 +64:24:43.1: 12.04 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:46:51.72 +64:24:43.1: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
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 20.1884* 09 46 51.72 +64 24 43.1 11.0 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
Gaia DR3 1064682878979387392,2461211.6884,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064682878979387392 20260620.1884 10.99CV 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 20.1884 2461211.6884 11.14 09:36:30.83 +65:23:05.3
147.53069 41.22807 galactic UMa Second-epoch detections are separated by 1.0" and 3.6 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 | Gaia DR3 1064949824082884608 | 09:36:30.86 +65:23:05.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.282+/-0.030 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:36:30.83 +65:23:05.3: 12.02 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:36:30.83 +65:23:05.3: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
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 20.1884* 09 36 30.83 +65 23 05.3 11.1 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
Gaia DR3 1064949824082884608,2461211.6884,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064949824082884608 20260620.1884 11.14CV 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 20.1884 2461211.6884 11.48 09:31:46.90 +64:43:00.5
148.61964 41.07671 galactic UMa Second-epoch detections are separated by 1.7" and 3.4 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 | Gaia DR3 1064531391189170688 | 09:31:47.14 +64:43:00.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.255+/-0.027 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:31:46.90 +64:43:00.5: 12.49 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:31:46.90 +64:43:00.5: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
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 20.1884* 09 31 46.90 +64 43 00.5 11.5 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
Gaia DR3 1064531391189170688,2461211.6884,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064531391189170688 20260620.1884 11.48CV 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 20.1884 2461211.6884 10.12 09:49:07.75 +64:57:45.5
147.17212 42.59191 galactic UMa Second-epoch detections are separated by 0.5" and 3.4 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 | Gaia DR3 1064735556753389824 | 09:49:07.58 +64:57:44.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.263+/-0.030 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:49:07.75 +64:57:45.5: 11.18 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:49:07.75 +64:57:45.5: 11.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
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 20.1884* 09 49 07.75 +64 57 45.5 10.1 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
Gaia DR3 1064735556753389824,2461211.6884,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064735556753389824 20260620.1884 10.12CV 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 20.1884 2461211.6884 10.98 09:42:56.31 +65:04:32.3
147.47416 41.96740 galactic UMa Second-epoch detections are separated by 1.0" and 3.5 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 | Gaia DR3 1064961643833013888 | 09:42:56.17 +65:04:31.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.299+/-0.028 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:42:56.31 +65:04:32.3: 11.96 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:42:56.31 +65:04:32.3: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
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 20.1884* 09 42 56.31 +65 04 32.3 11.0 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
Gaia DR3 1064961643833013888,2461211.6884,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064961643833013888 20260620.1884 10.98CV 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 20.1884 2461211.6884 11.44 09:44:05.93 +65:18:16.3
147.12555 41.96316 galactic UMa Second-epoch detections are separated by 2.3" and 3.1 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 | Gaia DR3 1064974460015400576 | 09:44:05.98 +65:18:16.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.587+/-0.026 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:44:05.93 +65:18:16.3: 12.44 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:44:05.93 +65:18:16.3: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
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 20.1884* 09 44 05.93 +65 18 16.3 11.4 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 1064974460015400576,2461211.6884,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064974460015400576 20260620.1884 11.44CV 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 20.1884 2461211.6884 10.87 09:44:43.87 +64:46:20.1
147.70910 42.28006 galactic UMa Second-epoch detections are separated by 0.6" and 3.4 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 | Gaia DR3 1064756069518264832 | 09:44:43.95 +64:46:19.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.347+/-0.028 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:44:43.87 +64:46:20.1: 11.92 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:44:43.87 +64:46:20.1: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
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 20.1884* 09 44 43.87 +64 46 20.1 10.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1064756069518264832,2461211.6884,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064756069518264832 20260620.1884 10.87CV 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 20.1884 2461211.6884 11.46 09:29:39.30 +65:43:26.0
147.54653 40.44175 galactic UMa Second-epoch detections are separated by 0.8" and 3.4 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 | Gaia DR3 1068007256682636416 | 09:29:39.24 +65:43:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.314+/-0.029 (F)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:29:39.30 +65:43:26.0: 12.44 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:29:39.30 +65:43:26.0: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
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 20.1884* 09 29 39.30 +65 43 26.0 11.5 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
Gaia DR3 1068007256682636416,2461211.6884,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1068007256682636416 20260620.1884 11.46CV 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 20.1884 2461211.6884 10.99 09:37:18.69 +65:08:00.3
147.77758 41.41724 galactic UMa Second-epoch detections are separated by 0.4" and 3.4 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 | Gaia DR3 1064930509614063616 | 09:37:18.74 +65:07:59.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.396+/-0.029 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:37:18.69 +65:08:00.3: 11.91 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:37:18.69 +65:08:00.3: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
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 20.1884* 09 37 18.69 +65 08 00.3 11.0 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
Gaia DR3 1064930509614063616,2461211.6884,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064930509614063616 20260620.1884 10.99CV 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 20.1884 2461211.6884 10.95 09:37:04.67 +65:06:47.3
147.81659 41.40464 galactic UMa Second-epoch detections are separated by 0.8" and 3.3 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 | Large-amplitude variable Gaia DR2 1064930372175111552 | 09:37:04.71 +65:06:46.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.446+/-0.030 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:37:04.67 +65:06:47.3: 11.90 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:37:04.67 +65:06:47.3: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
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 20.1884* 09 37 04.67 +65 06 47.3 10.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1064930372175111552,2461211.6884,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1064930372175111552 20260620.1884 10.95CV 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 20.1884 2461211.6884 11.41 09:37:16.79 +65:13:44.2
147.66640 41.37054 galactic UMa Second-epoch detections are separated by 2.0" and 3.2 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 | Gaia DR3 1064933297048755712 | 09:37:16.61 +65:13:43.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.360+/-0.029 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:37:16.79 +65:13:44.2: 12.44 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:37:16.79 +65:13:44.2: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
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 20.1884* 09 37 16.79 +65 13 44.2 11.4 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 1064933297048755712,2461211.6884,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064933297048755712 20260620.1884 11.41CV 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 20.1884 2461211.6884 10.98 09:41:21.44 +64:53:05.6
147.80663 41.91108 galactic UMa Second-epoch detections are separated by 1.3" and 3.5 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 | Gaia DR3 1064864818090165504 | 09:41:21.42 +64:53:05.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.547+/-0.027 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:41:21.44 +64:53:05.6: 11.90 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:41:21.44 +64:53:05.6: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
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 20.1884* 09 41 21.44 +64 53 05.6 11.0 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
Gaia DR3 1064864818090165504,2461211.6884,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064864818090165504 20260620.1884 10.98CV 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 20.1884 2461211.6884 10.96 09:33:31.31 +64:18:29.5
149.00314 41.42149 galactic UMa Second-epoch detections are separated by 0.8" and 3.4 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 | Gaia DR3 1064460850646288384 | 09:33:31.31 +64:18:28.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.615+/-0.028 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:33:31.31 +64:18:29.5: 11.88 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:33:31.31 +64:18:29.5: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
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 20.1884* 09 33 31.31 +64 18 29.5 11.0 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
Gaia DR3 1064460850646288384,2461211.6884,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064460850646288384 20260620.1884 10.96CV 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 20.1884 2461211.6884 11.54 09:30:26.71 +65:00:52.9
148.34365 40.82093 galactic UMa Second-epoch detections are separated by 2.5" and 3.1 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 | Gaia DR3 1067544907746946176 | 09:30:26.68 +65:00:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.417+/-0.027 (G)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:30:26.71 +65:00:52.9: 12.42 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:30:26.71 +65:00:52.9: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
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 20.1884* 09 30 26.71 +65 00 52.9 11.5 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
Gaia DR3 1067544907746946176,2461211.6884,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1067544907746946176 20260620.1884 11.54CV 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 20.1884 2461211.6884 10.89 09:42:49.35 +65:23:33.0
147.10906 41.80409 galactic UMa Second-epoch detections are separated by 2.7" and 3.7 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 | Gaia DR3 1064988100831539328 | 09:42:49.45 +65:23:33.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.571+/-0.030 (K)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:42:49.35 +65:23:33.0: 11.86 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:42:49.35 +65:23:33.0: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.01
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 20.1884* 09 42 49.35 +65 23 33.0 10.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1064988100831539328,2461211.6884,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1064988100831539328 20260620.1884 10.89CV 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: 2461082.80383981 11.02.2026 07:17:21.760 /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
First image: 2461082.80383981 11.02.2026 07:17:21.760 /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
Last image: 2461211.68856846 20.06.2026 04:31:22.315 /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
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: 5 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): 9017
Objects passed selection criteria: 8952
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 5408.25
Average stars matched: 5258.5 (97.2311 %)
Memory usage VmPeak: 114828 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jun 19 23:43:24 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: 2461082.80383981 11.02.2026 07:17:21.760 /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
First image: 2461082.80383981 11.02.2026 07:17:21.760 /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
Last image: 2461211.68856846 20.06.2026 04:31:22.315 /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 135
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.26
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: 18 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): 52376
Objects passed selection criteria: 52172
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 32735.2
Average stars matched: 31585.5 (96.4877 %)
Memory usage VmPeak: 153568 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jun 19 23:45:37 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
SExtractor catalog cache: saved UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.cat to cache
SExtractor catalog cache: saved UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.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: 2461211.68814543
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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits exists and is non-empty
Saving wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits to local_wcs_cache/
'wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits' -> 'local_wcs_cache/wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits'
wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits exists and is non-empty
Saving wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits to local_wcs_cache/
'wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits' -> 'local_wcs_cache/wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits'
wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits exists and is non-empty
Saving wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits to local_wcs_cache/
'wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits' -> 'local_wcs_cache/wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits'
wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits exists and is non-empty
Saving wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits to local_wcs_cache/
'wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits' -> 'local_wcs_cache/wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits (1st reference image)
verification OK: wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
Image size: 941.6'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: 08:34:18.681 +61:59:39.30 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-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits (1st new image)
verification OK: wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
Image size: 941.8'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:34:33.513 +61:59:34.59 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:34:18.681 +61:59:39.30
Second-epoch image center 08:34:33.513 +61:59:34.59
Angular distance between the image centers 0.0290 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits (2nd new image)
verification OK: wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
Image size: 941.8'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:34:32.870 +61:59:55.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:34:18.681 +61:59:39.30
Second-epoch image center 08:34:32.870 +61:59:55.21
Angular distance between the image centers 0.0281 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 08:34:33.513 +61:59:34.59
Second-epoch second image center 08:34:32.870 +61:59:55.21
Angular distance between the image centers 0.00586 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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits &> /tmp/tmp.zkv8Nk31BS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits &> /tmp/tmp.OuCp1KrNKD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits &> /tmp/tmp.7MVCh3wv2e
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits &> /tmp/tmp.6r6lXE5Qps
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits and wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits and wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat
Found non-empty wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits and wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat
The reference image (wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits) and catalog (wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat) found
'wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat' -> 'wcsmag.cat'
Read 9619 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 109.7413 to 148.5402 deg, Dec +55.4564 to +67.4105 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 109.7413 to 148.5402 deg, Dec 55.4564 to 67.4105 deg
Loaded 8845 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): 5406 out of 5707 total matches.
Matched with Tycho-2 5707 out of 9619 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.868250
a=0.000000 b=1.000000 c=22.868250
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.34
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9619 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 109.7413 to 148.5402 deg, Dec +55.4564 to +67.4105 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 109.7413 to 148.5402 deg, Dec 55.4564 to 67.4105 deg
Loaded 8845 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): 5406 out of 5707 total matches.
Matched with Tycho-2 5707 out of 9619 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits:
Forced-photometry filter: calibrated wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits -> calib.txt_param_ref_wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits (aperture=6.2)
Read 9596 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 109.7413 to 148.5398 deg, Dec +55.4564 to +67.4103 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 109.7413 to 148.5398 deg, Dec 55.4564 to 67.4103 deg
Loaded 8845 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): 5389 out of 5703 total matches.
Matched with Tycho-2 5703 out of 9596 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits:
Forced-photometry filter: calibrated wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits -> calib.txt_param_ref_wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
2.2 pix UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
2.8 pix fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
2.8 pix fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
2.2 pix wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
2.2 pix wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
Limiting magnitude estimates:
15.3 mag. UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
15.3 mag. UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
12.2 mag. fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
12.2 mag. fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
All-image limiting magnitude estimate: 12.2 (SNR ) 10.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zkv8Nk31BS (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits' -> 'wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
WCS_IMAGE_NAME=wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
WCS-calibrated image found: wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
Checking if the catalog wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits alredy exist and is non-empty...
Catalog wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
WCS catalog name: wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=686, passed=9619
Got 9619 stars (including 8917 good ones) from the SExtractor catalog wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat
util/solve_plate_with_UCAC5 got 9619 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 727 to 789 (Dec 55.5 to 67.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 9437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 789 (Dec 55.5 to 67.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 9436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 9436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits N_match=972 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.496 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.391 sigma_q4_arcsec=0.306 n_q1=221 n_q2=284 n_q3=180 n_q4=287 worst_quadrant_to_overall_ratio=1.307
The image catalog is written to wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits -region wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.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.OuCp1KrNKD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.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-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits' -> 'wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
WCS_IMAGE_NAME=wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
WCS-calibrated image found: wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
Checking if the catalog wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat corresponding to the image wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits alredy exist and is non-empty...
Catalog wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat corresponding to the image wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
WCS catalog name: wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=696, passed=9596
Got 9596 stars (including 8884 good ones) from the SExtractor catalog wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat
util/solve_plate_with_UCAC5 got 9596 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 727 to 789 (Dec 55.5 to 67.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 9342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 789 (Dec 55.5 to 67.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 9341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 9341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits N_match=975 sigma_overall_arcsec=0.363 sigma_q1_arcsec=0.498 sigma_q2_arcsec=0.377 sigma_q3_arcsec=0.368 sigma_q4_arcsec=0.281 n_q1=215 n_q2=294 n_q3=176 n_q4=290 worst_quadrant_to_overall_ratio=1.371
The image catalog is written to wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits -region wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.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.7MVCh3wv2e (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_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.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_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
WCS_IMAGE_NAME=wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
WCS-calibrated image found: wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
Checking if the catalog wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat corresponding to the image wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat corresponding to the image wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
WCS catalog name: wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=55, passed=1230
Got 1230 stars (including 1173 good ones) from the SExtractor catalog wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat
util/solve_plate_with_UCAC5 got 1230 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 1195 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 1196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 1196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits N_match=959 sigma_overall_arcsec=0.465 sigma_q1_arcsec=0.380 sigma_q2_arcsec=0.543 sigma_q3_arcsec=0.385 sigma_q4_arcsec=0.501 n_q1=187 n_q2=295 n_q3=113 n_q4=364 worst_quadrant_to_overall_ratio=1.169
The image catalog is written to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits -region wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.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.6r6lXE5Qps (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_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.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_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
WCS_IMAGE_NAME=wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
WCS-calibrated image found: wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
Checking if the catalog wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat corresponding to the image wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat corresponding to the image wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
WCS catalog name: wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=90, passed=1348
Got 1348 stars (including 1257 good ones) from the SExtractor catalog wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat
util/solve_plate_with_UCAC5 got 1348 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 1317 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 1316 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 1316 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits N_match=960 sigma_overall_arcsec=0.440 sigma_q1_arcsec=0.456 sigma_q2_arcsec=0.496 sigma_q3_arcsec=0.346 sigma_q4_arcsec=0.453 n_q1=175 n_q2=290 n_q3=122 n_q4=373 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits -region wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits sigma_overall=0.379 worst_q_ratio=1.307
ref2=UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits sigma_overall=0.363 worst_q_ratio=1.371
new1=fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits sigma_overall=0.465 worst_q_ratio=1.169
new2=fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits sigma_overall=0.440 worst_q_ratio=1.130
reference average sigma_overall=0.371 worst_q_ratio=1.339
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302_astrometric_residuals.png (972 matched stars from wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303_astrometric_residuals.png (975 matched stars from wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116_astrometric_residuals.png (959 matched stars from wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117_astrometric_residuals.png (960 matched stars from wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits'
Saving fully-calibrated image wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits'
Preparing the HTML report for the field UMa-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field UMa-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
SExtractor catalog cache: saved UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.cat to cache
SExtractor catalog cache: saved UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
Creating symlink local_wcs_cache/wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits exists and is non-empty
wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits exists and is non-empty
wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits exists and is non-empty
wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits (1st reference image)
verification OK: wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
Image size: 941.6'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: 08:34:18.681 +61:59:39.30 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-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits (1st new image)
verification OK: wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
Image size: 941.8'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:34:33.513 +61:59:34.59 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:34:18.681 +61:59:39.30
Second-epoch image center 08:34:33.513 +61:59:34.59
Angular distance between the image centers 0.0290 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits (2nd new image)
verification OK: wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
Image size: 941.8'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:34:32.870 +61:59:55.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:34:18.681 +61:59:39.30
Second-epoch image center 08:34:32.870 +61:59:55.21
Angular distance between the image centers 0.0281 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 08:34:33.513 +61:59:34.59
Second-epoch second image center 08:34:32.870 +61:59:55.21
Angular distance between the image centers 0.00586 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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits &> /tmp/tmp.c1Lqwi2S4Q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits &> /tmp/tmp.3Gizr7XpoE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits &> /tmp/tmp.HNsiCK3DOB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits &> /tmp/tmp.J4YeC1jWxO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits and wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits and wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat
Found non-empty wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits and wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat
The reference image (wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits) and catalog (wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat) found
'wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat' -> 'wcsmag.cat'
Read 56661 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 109.7413 to 148.5777 deg, Dec +55.3298 to +67.4117 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 109.7413 to 148.5777 deg, Dec 55.3298 to 67.4117 deg
Loaded 8951 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): 5042 out of 5784 total matches.
Matched with Tycho-2 5784 out of 56661 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.754150
a=0.000000 b=1.000000 c=22.754150
From vast_summary.log: estimated ref. image limiting mag.: -7.26
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 56661 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 109.7413 to 148.5777 deg, Dec +55.3298 to +67.4117 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 109.7413 to 148.5777 deg, Dec 55.3298 to 67.4117 deg
Loaded 8951 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): 5042 out of 5784 total matches.
Matched with Tycho-2 5784 out of 56661 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits:
Forced-photometry filter: calibrated wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits -> calib.txt_param_ref_wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits (aperture=4.8)
Read 56645 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 109.7413 to 148.5774 deg, Dec +55.3470 to +67.4190 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 109.7413 to 148.5774 deg, Dec 55.3470 to 67.4190 deg
Loaded 8945 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): 5051 out of 5777 total matches.
Matched with Tycho-2 5777 out of 56645 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits:
Forced-photometry filter: calibrated wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits -> calib.txt_param_ref_wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 103 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
2.0 pix UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
2.5 pix fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
2.5 pix fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
2.0 pix wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
2.0 pix wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
Limiting magnitude estimates:
15.5 mag. UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
15.5 mag. UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
12.5 mag. fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
12.5 mag. fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.c1Lqwi2S4Q (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.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-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits' -> 'wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
WCS_IMAGE_NAME=wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
WCS-calibrated image found: wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
Checking if the catalog wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits alredy exist and is non-empty...
Catalog wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits
WCS catalog name: wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=2986, passed=56640
Got 56640 stars (including 53554 good ones) from the SExtractor catalog wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat
util/solve_plate_with_UCAC5 got 56640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 726 to 789 (Dec 55.3 to 67.4)
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(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 55428 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 726 to 789 (Dec 55.3 to 67.4)
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: 970 matched stars entering correct_measured_positions(), 55427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 55427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 970 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits N_match=970 sigma_overall_arcsec=0.380 sigma_q1_arcsec=0.482 sigma_q2_arcsec=0.357 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.325 n_q1=217 n_q2=281 n_q3=181 n_q4=291 worst_quadrant_to_overall_ratio=1.266
The image catalog is written to wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits -region wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.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.3Gizr7XpoE (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.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-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits' -> 'wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
WCS_IMAGE_NAME=wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
WCS-calibrated image found: wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
Checking if the catalog wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat corresponding to the image wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits alredy exist and is non-empty...
Catalog wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat corresponding to the image wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits
WCS catalog name: wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=2922, passed=56624
Got 56624 stars (including 53608 good ones) from the SExtractor catalog wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat
util/solve_plate_with_UCAC5 got 56624 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 55261 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 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 55262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 55262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits N_match=972 sigma_overall_arcsec=0.404 sigma_q1_arcsec=0.537 sigma_q2_arcsec=0.393 sigma_q3_arcsec=0.403 sigma_q4_arcsec=0.332 n_q1=212 n_q2=284 n_q3=185 n_q4=291 worst_quadrant_to_overall_ratio=1.330
The image catalog is written to wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits -region wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.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.HNsiCK3DOB (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_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.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_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
WCS_IMAGE_NAME=wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
WCS-calibrated image found: wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
Checking if the catalog wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat corresponding to the image wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat corresponding to the image wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
WCS catalog name: wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=191, passed=9039
Got 9039 stars (including 8832 good ones) from the SExtractor catalog wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat
util/solve_plate_with_UCAC5 got 9039 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8800 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8799 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8799 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits N_match=960 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.362 sigma_q2_arcsec=0.513 sigma_q3_arcsec=0.398 sigma_q4_arcsec=0.513 n_q1=192 n_q2=296 n_q3=114 n_q4=358 worst_quadrant_to_overall_ratio=1.119
The image catalog is written to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits -region wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.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.J4YeC1jWxO (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_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.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_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
WCS_IMAGE_NAME=wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
WCS-calibrated image found: wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
Checking if the catalog wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat corresponding to the image wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat corresponding to the image wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
WCS catalog name: wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=167, passed=9555
Got 9555 stars (including 9364 good ones) from the SExtractor catalog wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat
util/solve_plate_with_UCAC5 got 9555 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 9350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 9351 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 9351 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits N_match=959 sigma_overall_arcsec=0.440 sigma_q1_arcsec=0.435 sigma_q2_arcsec=0.508 sigma_q3_arcsec=0.371 sigma_q4_arcsec=0.459 n_q1=184 n_q2=287 n_q3=121 n_q4=367 worst_quadrant_to_overall_ratio=1.155
The image catalog is written to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits -region wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.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-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.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_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-30-45_20.00sec_0.00C_LIGHTs_0116.fits
Saving fully-calibrated image wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.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_2026-06-19_CI_UMa-02-Q1b1x1_233448_TTUQ1b1x1_2582963_vzMf7n48/wcs_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117.fits
Preparing the HTML report for the field UMa-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:36:38.37 +56:58:34.5: 10.83 +/- 0.00 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:39:10.33 +56:40:47.8: 99.00 +/- 99.00 edge
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:36:19.37 +57:09:55.4: 11.40 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:37:35.71 +56:43:56.0: 11.02 +/- 0.00 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:35:31.82 +57:09:26.7: 11.43 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:37:12.91 +61:49:43.6: 11.04 +/- 0.00 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:35:31.50 +57:11:32.1: 11.16 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:38:35.92 +56:48:22.1: 11.53 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:36:38.39 +56:44:57.8: 11.88 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:39:10.33 +56:40:47.8: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 07:39:10.33 +56:40:47.8: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:36:19.37 +57:09:55.4: 11.40 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:36:38.37 +56:58:34.5: 10.82 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.40 +/- 0.00
Forced photometry filter REJECTED candidate at 07:36:19.37 +57:09:55.4: ref_mag=11.40 +/- 0.00 new_mean_mag=10.7798 delta=0.62 (need > 0.90)
Forced photometry reference-image weighted average: 10.82 +/- 0.00
Forced photometry filter REJECTED candidate at 07:36:38.37 +56:58:34.5: ref_mag=10.82 +/- 0.00 new_mean_mag=10.3950 delta=0.43 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:37:12.91 +61:49:43.6: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.00
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:35:31.82 +57:09:26.7: 11.46 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 07:37:12.91 +61:49:43.6: ref_mag=11.03 +/- 0.00 new_mean_mag=11.0549 delta=-0.02 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:37:35.71 +56:43:56.0: 11.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:35:31.50 +57:11:32.1: 11.15 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 07:35:31.82 +57:09:26.7: ref_mag=11.44 +/- 0.01 new_mean_mag=10.9046 delta=0.54 (need > 0.90)
Forced photometry reference-image weighted average: 11.04 +/- 0.00
Forced photometry filter REJECTED candidate at 07:37:35.71 +56:43:56.0: ref_mag=11.04 +/- 0.00 new_mean_mag=10.5363 delta=0.50 (need > 0.90)
Forced photometry reference-image weighted average: 11.16 +/- 0.00
Forced photometry filter REJECTED candidate at 07:35:31.50 +57:11:32.1: ref_mag=11.16 +/- 0.00 new_mean_mag=10.6956 delta=0.46 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:38:35.92 +56:48:22.1: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.01
Forced photometry filter REJECTED candidate at 07:38:35.92 +56:48:22.1: ref_mag=11.53 +/- 0.01 new_mean_mag=11.0103 delta=0.52 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:36:38.39 +56:44:57.8: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Forced photometry filter REJECTED candidate at 07:36:38.39 +56:44:57.8: ref_mag=11.88 +/- 0.01 new_mean_mag=11.4299 delta=0.45 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:36:01.38 +57:17:49.1: 12.23 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:35:33.64 +57:10:44.3: 12.21 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:36:19.58 +57:06:36.1: 12.48 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:36:01.38 +57:17:49.1: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Forced photometry filter REJECTED candidate at 07:36:01.38 +57:17:49.1: ref_mag=12.25 +/- 0.01 new_mean_mag=11.5419 delta=0.70 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:35:31.70 +57:28:53.1: 12.51 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:36:26.89 +57:05:35.6: 12.52 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:36:14.97 +56:59:44.5: 12.48 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:35:33.64 +57:10:44.3: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter REJECTED candidate at 07:35:33.64 +57:10:44.3: ref_mag=12.20 +/- 0.01 new_mean_mag=11.6557 delta=0.54 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:36:01.67 +57:10:47.9: 12.80 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:36:19.58 +57:06:36.1: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter REJECTED candidate at 07:36:19.58 +57:06:36.1: ref_mag=12.48 +/- 0.01 new_mean_mag=11.7647 delta=0.72 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:35:31.70 +57:28:53.1: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter REJECTED candidate at 07:35:31.70 +57:28:53.1: ref_mag=12.54 +/- 0.01 new_mean_mag=11.7526 delta=0.78 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:36:14.97 +56:59:44.5: 12.43 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:40:07.55 +56:42:49.3: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:36:49.44 +65:35:43.9: 12.04 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:36:26.89 +57:05:35.6: 12.47 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 07:36:14.97 +56:59:44.5: ref_mag=12.45 +/- 0.01 new_mean_mag=11.8213 delta=0.63 (need > 0.90)
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:38:08.61 +56:43:58.1: 12.77 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 07:36:26.89 +57:05:35.6: ref_mag=12.49 +/- 0.01 new_mean_mag=11.8087 delta=0.69 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:36:01.67 +57:10:47.9: 12.78 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Forced photometry filter REJECTED candidate at 07:36:01.67 +57:10:47.9: ref_mag=12.79 +/- 0.02 new_mean_mag=12.0727 delta=0.72 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:36:21.48 +56:49:28.7: 12.83 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:40:07.55 +56:42:49.3: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 07:40:07.55 +56:42:49.3: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:36:49.44 +65:35:43.9: 12.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.02
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:38:08.61 +56:43:58.1: 12.76 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 07:36:49.44 +65:35:43.9: ref_mag=12.02 +/- 0.02 new_mean_mag=11.9080 delta=0.12 (need > 0.90)
Forced photometry reference-image weighted average: 12.76 +/- 0.02
Forced photometry filter REJECTED candidate at 07:38:08.61 +56:43:58.1: ref_mag=12.76 +/- 0.02 new_mean_mag=12.1484 delta=0.62 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:36:40.92 +56:41:15.8: 12.96 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:36:21.48 +56:49:28.7: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry filter REJECTED candidate at 07:36:21.48 +56:49:28.7: ref_mag=12.81 +/- 0.02 new_mean_mag=12.1562 delta=0.66 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:45:16.75 +63:49:01.8: 12.27 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:30:43.08 +65:32:16.4: 11.45 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:32:25.64 +65:40:43.3: 12.79 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:36:40.92 +56:41:15.8: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter REJECTED candidate at 07:36:40.92 +56:41:15.8: ref_mag=12.98 +/- 0.02 new_mean_mag=12.2745 delta=0.71 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:44:16.47 +63:54:52.8: 11.86 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:46:13.84 +63:35:04.1: 12.37 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:47:33.28 +64:14:46.1: 11.84 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:45:16.75 +63:49:01.8: 12.25 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:34:09.52 +64:53:38.6: 11.81 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:31:38.67 +65:04:10.9: 11.80 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:30:43.08 +65:32:16.4: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 09:45:16.75 +63:49:01.8: ref_mag=12.26 +/- 0.01 new_mean_mag=11.2454 delta=1.01 (need > 0.90)
Forced photometry reference-image weighted average: 11.45 +/- 0.00
Forced photometry filter KEPT candidate at 09:30:43.08 +65:32:16.4: ref_mag=11.45 +/- 0.00 new_mean_mag=10.5375 delta=0.91 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:32:25.64 +65:40:43.3: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 09:32:25.64 +65:40:43.3: ref_mag=12.80 +/- 0.01 new_mean_mag=11.5909 delta=1.21 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:44:16.47 +63:54:52.8: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Forced photometry filter KEPT candidate at 09:44:16.47 +63:54:52.8: ref_mag=11.84 +/- 0.01 new_mean_mag=10.9309 delta=0.91 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:46:13.84 +63:35:04.1: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 09:46:13.84 +63:35:04.1: ref_mag=12.36 +/- 0.01 new_mean_mag=11.2895 delta=1.07 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:34:06.72 +64:42:35.1: 12.35 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:34:09.52 +64:53:38.6: 11.81 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:31:38.67 +65:04:10.9: 11.76 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:47:33.28 +64:14:46.1: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Forced photometry filter KEPT candidate at 09:34:09.52 +64:53:38.6: ref_mag=11.81 +/- 0.01 new_mean_mag=10.8750 delta=0.94 (need > 0.90)
Forced photometry filter KEPT candidate at 09:31:38.67 +65:04:10.9: ref_mag=11.78 +/- 0.01 new_mean_mag=10.8766 delta=0.90 (need > 0.90)
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Forced photometry filter KEPT candidate at 09:47:33.28 +64:14:46.1: ref_mag=11.85 +/- 0.01 new_mean_mag=10.8520 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:43:48.60 +63:39:24.0: 12.32 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:34:06.72 +64:42:35.1: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 09:34:06.72 +64:42:35.1: ref_mag=12.35 +/- 0.01 new_mean_mag=11.3450 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:43:48.60 +63:39:24.0: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter KEPT candidate at 09:43:48.60 +63:39:24.0: ref_mag=12.32 +/- 0.01 new_mean_mag=11.2755 delta=1.04 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:48:01.75 +64:47:03.5: 12.31 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:48:01.75 +64:47:03.5: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter KEPT candidate at 09:48:01.75 +64:47:03.5: ref_mag=12.33 +/- 0.01 new_mean_mag=11.0131 delta=1.32 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:46:54.02 +65:14:32.8: 10.56 +/- 0.00 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:30:26.20 +65:47:40.2: 12.26 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:46:54.02 +65:14:32.8: 10.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.57 +/- 0.00
Forced photometry filter KEPT candidate at 09:46:54.02 +65:14:32.8: ref_mag=10.57 +/- 0.00 new_mean_mag=9.6417 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:30:26.20 +65:47:40.2: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 09:30:26.20 +65:47:40.2: ref_mag=12.26 +/- 0.01 new_mean_mag=11.3035 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:43:42.57 +64:29:24.3: 12.25 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:33:49.67 +65:31:05.8: 12.20 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:43:42.57 +64:29:24.3: 12.24 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:42:12.74 +65:15:34.2: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Forced photometry filter KEPT candidate at 09:43:42.57 +64:29:24.3: ref_mag=12.25 +/- 0.01 new_mean_mag=11.2517 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:48:56.10 +64:42:51.0: 12.19 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:33:49.67 +65:31:05.8: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry filter KEPT candidate at 09:33:49.67 +65:31:05.8: ref_mag=12.21 +/- 0.01 new_mean_mag=10.9769 delta=1.24 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:39:50.17 +58:29:22.1: 13.24 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:45:55.68 +63:59:49.2: 12.16 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:42:12.74 +65:15:34.2: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.00
Forced photometry filter KEPT candidate at 09:42:12.74 +65:15:34.2: ref_mag=11.55 +/- 0.00 new_mean_mag=10.5580 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:48:56.10 +64:42:51.0: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter KEPT candidate at 09:48:56.10 +64:42:51.0: ref_mag=12.20 +/- 0.01 new_mean_mag=11.1280 delta=1.07 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:39:50.17 +58:29:22.1: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 07:39:50.17 +58:29:22.1: ref_mag=13.26 +/- 0.02 new_mean_mag=12.2799 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:45:55.68 +63:59:49.2: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter KEPT candidate at 09:45:55.68 +63:59:49.2: ref_mag=12.17 +/- 0.01 new_mean_mag=11.0993 delta=1.07 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:45:23.74 +64:12:43.8: 12.15 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:45:23.74 +64:12:43.8: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry filter KEPT candidate at 09:45:23.74 +64:12:43.8: ref_mag=12.14 +/- 0.01 new_mean_mag=11.0388 delta=1.10 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:46:06.21 +64:54:06.2: 12.94 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:46:06.21 +64:54:06.2: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 09:46:06.21 +64:54:06.2: ref_mag=12.94 +/- 0.02 new_mean_mag=11.5257 delta=1.42 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:44:07.45 +64:34:21.2: 11.45 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:44:07.45 +64:34:21.2: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.00
Forced photometry filter KEPT candidate at 09:44:07.45 +64:34:21.2: ref_mag=11.47 +/- 0.00 new_mean_mag=10.4938 delta=0.98 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:38:05.92 +57:29:04.4: 12.96 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:38:05.92 +57:29:04.4: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 07:38:05.92 +57:29:04.4: ref_mag=12.94 +/- 0.02 new_mean_mag=11.8960 delta=1.04 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:48:05.93 +64:33:09.2: 12.10 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:48:05.93 +64:33:09.2: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry filter KEPT candidate at 09:48:05.93 +64:33:09.2: ref_mag=12.07 +/- 0.01 new_mean_mag=11.0719 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:35:05.46 +58:01:16.0: 13.21 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:35:05.46 +58:01:16.0: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 07:35:05.46 +58:01:16.0: ref_mag=13.19 +/- 0.02 new_mean_mag=12.2367 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:48:44.91 +64:24:40.3: 11.38 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:48:44.91 +64:24:40.3: 11.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.37 +/- 0.00
Forced photometry filter KEPT candidate at 09:48:44.91 +64:24:40.3: ref_mag=11.37 +/- 0.00 new_mean_mag=10.3681 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:40:55.12 +65:30:23.3: 12.08 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:40:55.12 +65:30:23.3: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry filter KEPT candidate at 09:40:55.12 +65:30:23.3: ref_mag=12.06 +/- 0.01 new_mean_mag=11.0225 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:41:17.31 +57:07:53.0: 13.21 +/- 0.03 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:41:17.31 +57:07:53.0: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 07:41:17.31 +57:07:53.0: ref_mag=13.26 +/- 0.02 new_mean_mag=12.2318 delta=1.02 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:46:11.58 +64:26:22.4: 12.55 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:46:11.58 +64:26:22.4: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 09:46:11.58 +64:26:22.4: ref_mag=12.56 +/- 0.01 new_mean_mag=11.3975 delta=1.16 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:48:37.76 +64:35:51.8: 11.33 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:48:37.76 +64:35:51.8: 11.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.00
Forced photometry filter KEPT candidate at 09:48:37.76 +64:35:51.8: ref_mag=11.33 +/- 0.00 new_mean_mag=10.3750 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:46:33.88 +65:11:52.5: 12.52 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:46:33.88 +65:11:52.5: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter KEPT candidate at 09:46:33.88 +65:11:52.5: ref_mag=12.55 +/- 0.01 new_mean_mag=11.4441 delta=1.10 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:37:43.78 +64:21:46.1: 12.04 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:37:43.78 +64:21:46.1: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry filter KEPT candidate at 09:37:43.78 +64:21:46.1: ref_mag=12.04 +/- 0.01 new_mean_mag=11.0843 delta=0.96 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:41:29.85 +63:35:28.3: 12.52 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:41:29.85 +63:35:28.3: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter KEPT candidate at 09:41:29.85 +63:35:28.3: ref_mag=12.51 +/- 0.01 new_mean_mag=11.3898 delta=1.12 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:46:51.72 +64:24:43.1: 12.04 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:46:51.72 +64:24:43.1: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry filter KEPT candidate at 09:46:51.72 +64:24:43.1: ref_mag=12.05 +/- 0.01 new_mean_mag=10.9931 delta=1.06 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:36:30.83 +65:23:05.3: 12.02 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:31:46.90 +64:43:00.5: 12.49 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:36:30.83 +65:23:05.3: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry filter KEPT candidate at 09:36:30.83 +65:23:05.3: ref_mag=12.04 +/- 0.01 new_mean_mag=11.1222 delta=0.92 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:31:46.90 +64:43:00.5: 12.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter KEPT candidate at 09:31:46.90 +64:43:00.5: ref_mag=12.51 +/- 0.01 new_mean_mag=11.4740 delta=1.04 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:49:07.75 +64:57:45.5: 11.18 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:49:07.75 +64:57:45.5: 11.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Forced photometry filter KEPT candidate at 09:49:07.75 +64:57:45.5: ref_mag=11.17 +/- 0.00 new_mean_mag=10.1096 delta=1.06 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:42:56.31 +65:04:32.3: 11.96 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:42:56.31 +65:04:32.3: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Forced photometry filter KEPT candidate at 09:42:56.31 +65:04:32.3: ref_mag=11.96 +/- 0.01 new_mean_mag=10.9838 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:44:05.93 +65:18:16.3: 12.44 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:44:05.93 +65:18:16.3: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter KEPT candidate at 09:44:05.93 +65:18:16.3: ref_mag=12.43 +/- 0.01 new_mean_mag=11.4377 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:44:43.87 +64:46:20.1: 11.92 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:29:39.30 +65:43:26.0: 12.44 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:44:43.87 +64:46:20.1: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry filter KEPT candidate at 09:44:43.87 +64:46:20.1: ref_mag=11.90 +/- 0.01 new_mean_mag=10.8637 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:29:39.30 +65:43:26.0: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter KEPT candidate at 09:29:39.30 +65:43:26.0: ref_mag=12.45 +/- 0.01 new_mean_mag=11.4652 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:37:18.69 +65:08:00.3: 11.91 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:37:18.69 +65:08:00.3: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry filter KEPT candidate at 09:37:18.69 +65:08:00.3: ref_mag=11.90 +/- 0.01 new_mean_mag=10.9900 delta=0.91 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:37:04.67 +65:06:47.3: 11.90 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:37:04.67 +65:06:47.3: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry filter KEPT candidate at 09:37:04.67 +65:06:47.3: ref_mag=11.90 +/- 0.01 new_mean_mag=10.9507 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:37:16.79 +65:13:44.2: 12.44 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:37:16.79 +65:13:44.2: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter KEPT candidate at 09:37:16.79 +65:13:44.2: ref_mag=12.43 +/- 0.01 new_mean_mag=11.4013 delta=1.03 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:41:21.44 +64:53:05.6: 11.90 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:41:21.44 +64:53:05.6: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter KEPT candidate at 09:41:21.44 +64:53:05.6: ref_mag=11.92 +/- 0.01 new_mean_mag=10.9728 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 07:38:15.36 +57:44:23.2: 12.60 +/- 0.02 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 07:38:15.36 +57:44:23.2: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter REJECTED candidate at 07:38:15.36 +57:44:23.2: ref_mag=12.61 +/- 0.01 new_mean_mag=11.9561 delta=0.65 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:30:26.71 +65:00:52.9: 12.42 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:33:31.31 +64:18:29.5: 11.88 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:30:26.71 +65:00:52.9: 12.46 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:33:31.31 +64:18:29.5: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter KEPT candidate at 09:30:26.71 +65:00:52.9: ref_mag=12.44 +/- 0.01 new_mean_mag=11.4555 delta=0.99 (need > 0.90)
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Forced photometry filter KEPT candidate at 09:33:31.31 +64:18:29.5: ref_mag=11.88 +/- 0.01 new_mean_mag=10.9413 delta=0.94 (need > 0.90)
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-17-21_20.00sec_-14.90C_LIGHT_0302.fits at 09:42:49.35 +65:23:33.0: 11.86 +/- 0.01 detection
Forced photometry on wcs_UMa-02-Q1b1x1_2026-02-11_01-18-03_20.00sec_-15.00C_LIGHT_0303.fits at 09:42:49.35 +65:23:33.0: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.01
Forced photometry filter KEPT candidate at 09:42:49.35 +65:23:33.0: ref_mag=11.86 +/- 0.01 new_mean_mag=10.8669 delta=0.99 (need > 0.90)
Adding exclusion_list_local.txt__out01036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46238.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 85s
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: 25s
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Considering the candidate 70754_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70754_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70757_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70757_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 07:36:48.54 +56:51:27.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 70763_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70763_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 70771_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70771_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 70782_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70782_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70788_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70788_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70793_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70793_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70799_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70799_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70806_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70806_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70814_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70814_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70823_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70823_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70829_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70829_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 70842_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70842_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70849_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70849_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 08:30:26.59 +60:41:08.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 70872_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70872_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70894_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70894_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70915_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70915_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70921_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70921_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 09:31:19.76 +63:02:40.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 70926_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70926_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70934_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70934_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 08:30:06.27 +60:40:34.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 70936_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70936_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70941_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70941_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 70945_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70945_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70961_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70961_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70962_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70962_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70975_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70975_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70983_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70983_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 70987_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 70987_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 71014_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 71014_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 71053_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 71053_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 71082_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 71082_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 02640_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 02640_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 08296_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 08296_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 01803_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 01803_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 08023_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 08023_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 09260_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 09260_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 05668_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 05668_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 05170_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 05170_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 04780_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 04780_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 06158_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 06158_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 09395_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 09395_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 03067_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 03067_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 01036_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 01036_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 01526_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 01526_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 05324_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 05324_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 02243_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 02243_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 01953_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 01953_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 03218_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 03218_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 07287_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 07287_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 46238_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 46238_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 06311_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 06311_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 02946_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 02946_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 04787_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 04787_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 38582_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 38582_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 04138_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 04138_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 44124_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 44124_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 04610_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 04610_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 01057_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 01057_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 36488_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 36488_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 05069_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 05069_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03785_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 03785_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01399_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 01399_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07138_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 07138_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10206_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 10206_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05031_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 05031_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17952_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 17952_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 09:36:44.24 +62:17:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02453_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 02453_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06568_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 06568_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01925_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 01925_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02707_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 02707_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01412_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 01412_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03805_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 03805_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02019_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 02019_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03490_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 03490_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03628_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 03628_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03061_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 03061_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03945_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 03945_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40605_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 40605_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36104_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 36104_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 07:55:51.00 +57:11:54.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08226_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 08226_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05286_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 05286_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02046_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 02046_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 09:48:46.95 +64:53:40.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39240_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 39240_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 08:30:15.48 +60:43:05.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25718_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 25718_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 08:19:17.27 +62:30:26.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26015_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 26015_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 08:53:22.48 +61:57:45.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14329_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 14329_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 08:40:12.53 +64:19:39.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10807_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 10807_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 08:39:11.57 +65:01:16.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10368_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 10368_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 08:34:35.95 +65:08:39.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11502_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 11502_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 08:56:37.19 +64:36:11.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08312_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 08312_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 09:45:55.32 +63:39:10.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15255_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 15255_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 09:10:55.22 +63:30:47.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41435_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 41435_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 08:20:26.35 +57:44:36.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02451_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 02451_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 09:44:36.44 +64:59:03.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26512_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 26512_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 09:14:20.37 +61:25:22.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43769_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 43769_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 08:10:03.78 +58:14:52.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36179_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 36179_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 07:40:49.64 +57:04:59.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10935_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 10935_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 09:25:44.09 +63:56:25.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39140_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 39140_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 08:01:20.98 +59:02:51.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42851_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 42851_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 09:21:43.04 +56:41:57.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01185_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 01185_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41929_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 41929_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 09:15:49.63 +56:44:28.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14174_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 14174_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 09:31:31.74 +63:03:43.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39758_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117
The candidate 39758_fd_UMa-02-Q1b1x1_2026-06-19_23-31-22_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 07:43:00.32 +58:42:37.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 113s
Prepared the HTML report for the field UMa-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:46:54.02 +65:14:32.8
09:40:55.12 +65:30:23.3
09:42:49.35 +65:23:33.0
09:46:33.88 +65:11:52.5
09:44:05.93 +65:18:16.3
09:30:26.20 +65:47:40.2
09:32:25.64 +65:40:43.3
09:49:07.75 +64:57:45.5
09:42:12.74 +65:15:34.2
09:29:39.30 +65:43:26.0
09:33:49.67 +65:31:05.8
09:36:30.83 +65:23:05.3
09:30:43.08 +65:32:16.4
09:42:56.31 +65:04:32.3
09:46:06.21 +64:54:06.2
09:37:16.79 +65:13:44.2
09:48:01.75 +64:47:03.5
09:48:56.10 +64:42:51.0
09:37:18.69 +65:08:00.3
09:37:04.67 +65:06:47.3
09:48:37.76 +64:35:51.8
09:44:43.87 +64:46:20.1
09:41:21.44 +64:53:05.6
09:48:05.93 +64:33:09.2
09:48:44.91 +64:24:40.3
09:31:38.67 +65:04:10.9
09:44:07.45 +64:34:21.2
09:46:51.72 +64:24:43.1
09:46:11.58 +64:26:22.4
09:34:09.52 +64:53:38.6
09:30:26.71 +65:00:52.9
09:43:42.57 +64:29:24.3
09:47:33.28 +64:14:46.1
09:34:06.72 +64:42:35.1
09:45:23.74 +64:12:43.8
09:31:46.90 +64:43:00.5
09:37:43.78 +64:21:46.1
09:45:55.68 +63:59:49.2
09:44:16.47 +63:54:52.8
09:33:31.31 +64:18:29.5
09:45:16.75 +63:49:01.8
09:46:13.84 +63:35:04.1
09:43:48.60 +63:39:24.0
09:41:29.85 +63:35:28.3
07:41:17.31 +57:07:53.0
07:38:05.92 +57:29:04.4
07:35:05.46 +58:01:16.0
07:39:50.17 +58:29:22.1
########### Completed UMa-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
09:30:43.08 +65:32:16.4
09:45:16.75 +63:49:01.8
09:32:25.64 +65:40:43.3
09:44:16.47 +63:54:52.8
09:46:13.84 +63:35:04.1
09:47:33.28 +64:14:46.1
09:34:09.52 +64:53:38.6
09:31:38.67 +65:04:10.9
09:34:06.72 +64:42:35.1
09:43:48.60 +63:39:24.0
09:48:01.75 +64:47:03.5
09:46:54.02 +65:14:32.8
09:30:26.20 +65:47:40.2
09:43:42.57 +64:29:24.3
09:33:49.67 +65:31:05.8
09:42:12.74 +65:15:34.2
09:48:56.10 +64:42:51.0
09:45:55.68 +63:59:49.2
07:39:50.17 +58:29:22.1
09:45:23.74 +64:12:43.8
09:46:06.21 +64:54:06.2
09:44:07.45 +64:34:21.2
07:38:05.92 +57:29:04.4
09:48:05.93 +64:33:09.2
07:35:05.46 +58:01:16.0
09:48:44.91 +64:24:40.3
09:40:55.12 +65:30:23.3
07:41:17.31 +57:07:53.0
09:46:11.58 +64:26:22.4
09:48:37.76 +64:35:51.8
09:46:33.88 +65:11:52.5
09:37:43.78 +64:21:46.1
09:41:29.85 +63:35:28.3
09:46:51.72 +64:24:43.1
09:36:30.83 +65:23:05.3
09:31:46.90 +64:43:00.5
09:49:07.75 +64:57:45.5
09:42:56.31 +65:04:32.3
09:44:05.93 +65:18:16.3
09:44:43.87 +64:46:20.1
09:29:39.30 +65:43:26.0
09:37:18.69 +65:08:00.3
09:37:04.67 +65:06:47.3
09:37:16.79 +65:13:44.2
09:41:21.44 +64:53:05.6
09:33:31.31 +64:18:29.5
09:30:26.71 +65:00:52.9
09:42:49.35 +65:23:33.0
###################################################################################
09:30:43.08 +65:32:16.4 -- not an asteroid (will add it to exclusion list)
09:45:16.75 +63:49:01.8 -- not an asteroid (will add it to exclusion list)
09:32:25.64 +65:40:43.3 -- not an asteroid (will add it to exclusion list)
09:44:16.47 +63:54:52.8 -- not an asteroid (will add it to exclusion list)
09:46:13.84 +63:35:04.1 -- not an asteroid (will add it to exclusion list)
09:47:33.28 +64:14:46.1 -- not an asteroid (will add it to exclusion list)
09:34:09.52 +64:53:38.6 -- not an asteroid (will add it to exclusion list)
09:31:38.67 +65:04:10.9 -- not an asteroid (will add it to exclusion list)
09:34:06.72 +64:42:35.1 -- not an asteroid (will add it to exclusion list)
09:43:48.60 +63:39:24.0 -- not an asteroid (will add it to exclusion list)
09:48:01.75 +64:47:03.5 -- not an asteroid (will add it to exclusion list)
09:46:54.02 +65:14:32.8 -- not an asteroid (will add it to exclusion list)
09:30:26.20 +65:47:40.2 -- not an asteroid (will add it to exclusion list)
09:43:42.57 +64:29:24.3 -- not an asteroid (will add it to exclusion list)
09:33:49.67 +65:31:05.8 -- not an asteroid (will add it to exclusion list)
09:42:12.74 +65:15:34.2 -- not an asteroid (will add it to exclusion list)
09:48:56.10 +64:42:51.0 -- not an asteroid (will add it to exclusion list)
09:45:55.68 +63:59:49.2 -- not an asteroid (will add it to exclusion list)
07:39:50.17 +58:29:22.1 -- not an asteroid (will add it to exclusion list)
09:45:23.74 +64:12:43.8 -- not an asteroid (will add it to exclusion list)
09:46:06.21 +64:54:06.2 -- not an asteroid (will add it to exclusion list)
09:44:07.45 +64:34:21.2 -- not an asteroid (will add it to exclusion list)
07:38:05.92 +57:29:04.4 -- not an asteroid (will add it to exclusion list)
09:48:05.93 +64:33:09.2 -- not an asteroid (will add it to exclusion list)
07:35:05.46 +58:01:16.0 -- not an asteroid (will add it to exclusion list)
09:48:44.91 +64:24:40.3 -- not an asteroid (will add it to exclusion list)
09:40:55.12 +65:30:23.3 -- not an asteroid (will add it to exclusion list)
07:41:17.31 +57:07:53.0 -- not an asteroid (will add it to exclusion list)
09:46:11.58 +64:26:22.4 -- not an asteroid (will add it to exclusion list)
09:48:37.76 +64:35:51.8 -- not an asteroid (will add it to exclusion list)
09:46:33.88 +65:11:52.5 -- not an asteroid (will add it to exclusion list)
09:37:43.78 +64:21:46.1 -- not an asteroid (will add it to exclusion list)
09:41:29.85 +63:35:28.3 -- not an asteroid (will add it to exclusion list)
09:46:51.72 +64:24:43.1 -- not an asteroid (will add it to exclusion list)
09:36:30.83 +65:23:05.3 -- not an asteroid (will add it to exclusion list)
09:31:46.90 +64:43:00.5 -- not an asteroid (will add it to exclusion list)
09:49:07.75 +64:57:45.5 -- not an asteroid (will add it to exclusion list)
09:42:56.31 +65:04:32.3 -- not an asteroid (will add it to exclusion list)
09:44:05.93 +65:18:16.3 -- not an asteroid (will add it to exclusion list)
09:44:43.87 +64:46:20.1 -- not an asteroid (will add it to exclusion list)
09:29:39.30 +65:43:26.0 -- not an asteroid (will add it to exclusion list)
09:37:18.69 +65:08:00.3 -- not an asteroid (will add it to exclusion list)
09:37:04.67 +65:06:47.3 -- not an asteroid (will add it to exclusion list)
09:37:16.79 +65:13:44.2 -- not an asteroid (will add it to exclusion list)
09:41:21.44 +64:53:05.6 -- not an asteroid (will add it to exclusion list)
09:33:31.31 +64:18:29.5 -- not an asteroid (will add it to exclusion list)
09:30:26.71 +65:00:52.9 -- not an asteroid (will add it to exclusion list)
09:42:49.35 +65:23:33.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
07:35:05.46 +58:01:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:05.92 +57:29:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:50.17 +58:29:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:17.31 +57:07:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:39.30 +65:43:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:30:26.20 +65:47:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:30:26.71 +65:00:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:30:43.08 +65:32:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:38.67 +65:04:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:46.90 +64:43:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:32:25.64 +65:40:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:33:31.31 +64:18:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:33:49.67 +65:31:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:34:06.72 +64:42:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:34:09.52 +64:53:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:36:30.83 +65:23:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:37:04.67 +65:06:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:37:16.79 +65:13:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:37:18.69 +65:08:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:37:43.78 +64:21:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:40:55.12 +65:30:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:41:21.44 +64:53:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:41:29.85 +63:35:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:42:12.74 +65:15:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:42:49.35 +65:23:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:42:56.31 +65:04:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:43:42.57 +64:29:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:43:48.60 +63:39:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:44:05.93 +65:18:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:44:07.45 +64:34:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:44:16.47 +63:54:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:44:43.87 +64:46:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:45:16.75 +63:49:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:45:23.74 +64:12:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:45:55.68 +63:59:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:46:06.21 +64:54:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:46:11.58 +64:26:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:46:13.84 +63:35:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:46:33.88 +65:11:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:46:51.72 +64:24:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:46:54.02 +65:14:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:47:33.28 +64:14:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:01.75 +64:47:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:05.93 +64:33:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:37.76 +64:35:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:44.91 +64:24:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:56.10 +64:42:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:49:07.75 +64:57:45.5 -- 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)
07:35:05.46 +58:01:16.0 -- not a known variable star
07:38:05.92 +57:29:04.4 -- not a known variable star
07:39:50.17 +58:29:22.1 -- not a known variable star
07:41:17.31 +57:07:53.0 -- not a known variable star
09:29:39.30 +65:43:26.0 -- not a known variable star
09:30:26.20 +65:47:40.2 -- not a known variable star
09:30:26.71 +65:00:52.9 -- not a known variable star
09:30:43.08 +65:32:16.4 -- not a known variable star
09:31:38.67 +65:04:10.9 -- not a known variable star
09:31:46.90 +64:43:00.5 -- not a known variable star
09:32:25.64 +65:40:43.3 -- a known variable star
09:33:31.31 +64:18:29.5 -- not a known variable star
09:33:49.67 +65:31:05.8 -- a known variable star
09:34:06.72 +64:42:35.1 -- not a known variable star
09:34:09.52 +64:53:38.6 -- not a known variable star
09:36:30.83 +65:23:05.3 -- not a known variable star
09:37:04.67 +65:06:47.3 -- not a known variable star
09:37:16.79 +65:13:44.2 -- not a known variable star
09:37:18.69 +65:08:00.3 -- not a known variable star
09:37:43.78 +64:21:46.1 -- not a known variable star
09:40:55.12 +65:30:23.3 -- not a known variable star
09:41:21.44 +64:53:05.6 -- not a known variable star
09:41:29.85 +63:35:28.3 -- not a known variable star
09:42:12.74 +65:15:34.2 -- not a known variable star
09:42:49.35 +65:23:33.0 -- not a known variable star
09:42:56.31 +65:04:32.3 -- not a known variable star
09:43:42.57 +64:29:24.3 -- not a known variable star
09:43:48.60 +63:39:24.0 -- not a known variable star
09:44:05.93 +65:18:16.3 -- not a known variable star
09:44:07.45 +64:34:21.2 -- not a known variable star
09:44:16.47 +63:54:52.8 -- not a known variable star
09:44:43.87 +64:46:20.1 -- not a known variable star
09:45:16.75 +63:49:01.8 -- not a known variable star
09:45:23.74 +64:12:43.8 -- not a known variable star
09:45:55.68 +63:59:49.2 -- not a known variable star
09:46:06.21 +64:54:06.2 -- not a known variable star
09:46:11.58 +64:26:22.4 -- not a known variable star
09:46:13.84 +63:35:04.1 -- not a known variable star
09:46:33.88 +65:11:52.5 -- not a known variable star
09:46:51.72 +64:24:43.1 -- not a known variable star
09:46:54.02 +65:14:32.8 -- not a known variable star
09:47:33.28 +64:14:46.1 -- not a known variable star
09:48:01.75 +64:47:03.5 -- not a known variable star
09:48:05.93 +64:33:09.2 -- not a known variable star
09:48:37.76 +64:35:51.8 -- not a known variable star
09:48:44.91 +64:24:40.3 -- not a known variable star
09:48:56.10 +64:42:51.0 -- not a known variable star
09:49:07.75 +64:57:45.5 -- not a known variable star
Found 46 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
48 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 48 (excluding asteroids and hot pixels, 46 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461211.68814543 -observatory V36
07:37:11.89 +21:44:19.1 Mercury (0.9mag)
08:41:34.09 +20:20:16.3 Venus (-4.0mag)
03:24:38.62 +18:13:02.8 Mars (1.3mag)
07:58:40.44 +21:04:32.9 Jupiter (-1.8mag)
00:52:26.46 +03:04:53.9 Saturn (0.8mag)
04:02:59.74 +20:33:23.2 Uranus (5.8mag)
00:16:42.56 +00:19:48.5 Neptune (7.8mag)
20:32:35.29 -23:09:17.8 Pluto (14.5mag)
10:32:53.00 +07:46:21.9 Moon (-9.8mag)
-rw-r--r-- 1 apache apache 361 Jun 19 23:43 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461211.68814543:
07:58:35.16 +21:04:50.6 Io (6.2mag)
07:58:49.76 +21:04:01.7 Europa (6.3mag)
07:58:51.19 +21:03:54.2 Ganymede (5.6mag)
07:59:01.61 +21:03:30.0 Callisto (6.9mag)
07:58:15.36 +20:42:27.9 Himalia (15.6mag)
07:58:42.05 +21:04:28.3 Thebe (16.6mag)
07:57:55.34 +20:52:58.7 Elara (17.6mag)
08:01:26.04 +21:09:41.0 Pasiphae (17.8mag)
08:04:42.20 +21:07:16.0 Carme (18.9mag)
00:52:21.69 +03:05:23.3 Titan (8.6mag)
00:52:31.68 +03:04:53.8 Rhea (9.9mag)
00:52:40.83 +03:07:17.5 Iapetus (11.3mag)
00:52:30.82 +03:05:21.3 Hyperion (14.6mag)
00:52:53.69 +03:05:05.6 Phoebe (16.6mag)
-rw-r--r-- 1 apache apache 568 Jun 19 23:43 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461211.68814543:
17:29:25.16 -35:32:13.3 JWST
18:25:20.08 +28:27:36.2 Chandra
19:00:33.98 -11:03:49.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 19 23:43 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461211.68814543 -observatory V36
18:34:26.66 -33:27:28.9 13.6mag P/2010 H2 (Vales)
06:05:24.03 -67:59:42.2 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
05:53:30.04 +32:07:56.2 17.6mag C/2017 K2 (PANSTARRS)
17:09:59.45 +15:49:24.7 17.9mag C/2021 G2 (ATLAS)
23:11:24.08 -36:22:06.7 15.9mag P/2021 N1 (ZTF)
23:09:09.85 +31:59:28.0 17.2mag C/2022 E2 (ATLAS)
05:48:38.76 +27:00:44.1 16.6mag C/2022 N2 (PANSTARRS)
09:38:46.01 +30:38:05.9 16.7mag C/2022 QE78 (ATLAS)
08:57:17.01 +04:26:17.4 17.7mag C/2022 R6 (PANSTARRS)
18:20:16.72 +21:42:12.4 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:15:31.17 -11:04:14.2 17.6mag P/2023 B1 (PANSTARRS)
22:08:24.30 +67:10:22.2 17.8mag C/2023 H5 (Lemmon)
17:16:33.76 -07:55:14.8 13.7mag C/2023 R1 (PANSTARRS)
13:17:34.55 +80:10:40.0 18.0mag C/2023 X2 (Lemmon)
07:27:52.44 +64:45:23.2 17.8mag C/2024 A1 (ATLAS)
07:05:01.74 +28:47:35.4 14.0mag C/2024 E1 (Wierzchos)
15:28:22.22 +14:25:50.4 17.4mag C/2024 G6 (ATLAS)
20:03:35.18 +34:34:33.6 13.9mag C/2024 J3 (ATLAS)
04:30:00.82 -14:59:24.5 15.9mag C/2024 T5 (ATLAS)
06:16:58.19 +32:26:18.9 17.9mag C/2025 J1 (Borisov)
11:32:04.47 +52:00:58.5 17.8mag C/2025 L1 (ATLAS)
06:57:49.75 -11:27:49.1 15.1mag C/2025 R3 (PANSTARRS)
09:34:47.65 +23:06:49.6 17.8mag C/2025 V2 (Rankin)
12:40:11.82 +04:33:29.0 17.1mag C/2025 Y1 (ATLAS)
17:48:46.20 +77:21:27.3 17.7mag C/2026 A2 (Bok)
02:20:09.34 +44:12:01.4 16.3mag C/2026 B2 (Sun-Gao)
11:14:57.92 +00:01:17.7 16.6mag A/2026 E1
20:45:06.99 -09:55:54.5 8.1mag 10P/Tempel
11:05:23.43 -01:12:15.1 16.0mag 29P/Schwassmann-Wachmann
03:30:09.46 +27:11:48.0 17.7mag 47P/Ashbrook-Jackson
09:25:32.33 +20:15:23.8 16.9mag 63P/Wild
00:36:27.36 -05:41:56.9 15.6mag 65P/Gunn
07:22:25.63 +34:17:16.0 17.2mag 76P/West-Kohoutek-Ikemura
03:38:18.27 +18:35:57.3 13.8mag 78P/Gehrels
01:45:44.02 +07:17:30.5 15.8mag 88P/Howell
05:33:06.00 +30:53:41.5 15.4mag 93P/Lovas
03:17:54.76 +29:21:13.9 17.3mag 114P/Wiseman-Skiff
07:19:26.30 +32:26:41.6 15.5mag 123P/West-Hartley
10:11:20.20 +09:32:34.4 16.6mag 124P/Mrkos
04:18:49.44 +19:58:25.4 16.3mag 128P/Shoemaker-Holt
04:57:18.03 +19:31:05.2 17.8mag 131P/Mueller
06:46:46.82 +16:58:08.2 16.2mag 141P/Machholz
06:50:20.94 +17:52:33.2 16.1mag 141P-A/Machholz
05:52:11.41 +17:16:51.6 13.0mag 141P-D/Machholz
03:05:46.93 -23:09:18.1 16.4mag 161P/Hartley-IRAS
04:21:52.11 +28:16:16.9 15.0mag 162P/SidingSpring
19:32:39.19 +05:39:41.7 16.2mag 169P/NEAT
00:50:13.58 +04:40:47.5 17.8mag 220P/McNaught
16:43:49.50 -08:06:10.8 16.6mag 235P/LINEAR
08:01:32.96 +34:51:55.6 17.7mag 240P/NEAT
01:04:08.37 +02:46:49.0 16.1mag 260P/McNaught
04:37:40.21 +34:28:35.8 17.5mag 295P/LINEAR
00:54:41.62 +03:09:47.6 17.9mag 320P/McNaught
15:10:33.39 +07:32:48.4 17.5mag 391P/Kowalski
08:16:59.30 +20:24:12.2 17.9mag 450P/LONEOS
07:19:29.80 +40:49:00.1 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 19 23:43 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
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
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
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
15:03:05.18 +22:02:03.40 AT2026lxf 2026-05-8.07 13.94
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
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
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
20:49:13.39 +25:17:59.20 2026-06-15.39 15.93
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
14:49:14.01 -27:29:20.10 ASASSN-26cu 2026-04-16.29 -2.7
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
20:49:13.39 +25:17:59.20 2026-06-15.39 15.93
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 2026-04-9.14 13.64
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
19:32:43.68 -22:39:32.70 ASASSN-26cm 2026-04-4.27 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
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
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
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
-rw-r--r-- 1 apache apache 5.6K Jun 19 23:43 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
-rw-r--r-- 1 apache apache 189K Jun 19 23:43 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:39:23.496 +35:21:27.84 AT 2026oxy 2026-06-04.97 20.13
23:44:57.556 +04:18:42.85 SN 2026oxx 2026-06-11.15 19.97
15:19:13.587 +27:52:58.57 SN 2026oxw 2026-06-11.02 19.96
09:53:09.311 +42:13:35.56 AT 2026oxv 2026-06-10.17 19.7446
20:30:02.168 +37:49:06.79 AT 2026oxu 2026-06-10.94 19.78
16:00:10.377 +22:09:10.94 AT 2026oxt 2026-06-11.03 19.379
17:32:05.150 +18:24:04.24 AT 2026oxs 2026-06-11.07 20.323
16:01:14.849 +29:49:20.54 AT 2026oxr 2026-06-08.41 18.733
18:33:36.042 +54:00:37.60 AT 2026oxq 2026-06-10.04 19.165
16:26:58.974 +50:28:07.45 AT 2026oxp 2026-06-10.01 20.192
19:48:49.856 +70:58:44.48 SN 2026oxo 2026-06-10.06 19.319
12:22:13.437 +27:24:59.57 AT 2026oxn 2026-06-10.94 19.381
23:01:57.544 -22:53:59.27 AT 2026oxm 2026-06-10.56 18.766
23:50:06.038 -14:01:39.26 AT 2026oxl 2026-06-10.58 18.422
13:13:55.656 -30:49:07.21 AT 2026oxk 2026-06-11.21 19.115
19:13:25.854 +49:32:53.84 AT 2026oxj 2026-06-10.06 19.005
23:31:30.736 +31:22:08.82 AT 2026oxi 2026-06-11.17 18.865
21:36:15.644 -21:19:14.62 AT 2026oxh 2026-06-10.53 18.749
22:37:33.079 +29:47:40.75 AT 2026oxg 2026-06-11.14 19.184
20:53:38.599 -35:13:40.58 SN 2026oxf 2026-06-10.52 18.812
-rw-r--r-- 1 apache apache 30K Jun 19 23:43 tns_transients_list.txt
