This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy
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 09 15.3628 2461298.8629 12.93 09:18:33.47 +68:41:51.1
144.66406 38.20069 galactic UMa Second-epoch detections are separated by 2.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:18:33.47 +68:41:51.1 (user input) | T | P | (position from user input) J-Ks=0.555+/-0.030 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:18:33.47 +68:41:51.1: 13.82 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:18:33.47 +68:41:51.1: 13.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 18 33.47 +68 41 51.1 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.93,0.05,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
target 20260915.3628 12.93CV 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 09 15.3628 2461298.8629 12.93 09:26:23.20 +67:35:20.9
145.54395 39.33580 galactic UMa Second-epoch detections are separated by 2.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:26:23.20 +67:35:20.9 (user input) | T | P | (position from user input) J-Ks=0.465+/-0.031 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:26:23.20 +67:35:20.9: 13.85 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:26:23.20 +67:35:20.9: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 26 23.20 +67 35 20.9 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.93,0.05,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
target 20260915.3628 12.93CV 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 09 15.3628 2461298.8629 12.87 10:35:48.89 +74:00:32.5
134.49207 39.92823 galactic Dra Second-epoch detections are separated by 1.6" and 5.7 pix
The object was found in VSX 1" Gaia DR3 1078394720986722688
Type: ROT
# Max. Min./Amp. JD0 Period
13.670 G 13.700 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:35:48.89 +74:00:32.5: 13.87 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:35:48.89 +74:00:32.5: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1078394720986722688,2461298.8629,12.87,0.05,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 1078394720986722688 20260915.3628 12.87CV 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 09 15.3628 2461298.8629 12.93 09:41:17.54 +69:40:53.4
142.32430 39.51271 galactic UMa Second-epoch detections are separated by 0.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:41:17.54 +69:40:53.4 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.034 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:41:17.54 +69:40:53.4: 13.94 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:41:17.54 +69:40:53.4: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 41 17.54 +69 40 53.4 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.93,0.05,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
target 20260915.3628 12.93CV 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 09 15.3628 2461298.8629 13.04 09:43:31.50 +69:08:03.6
142.79465 39.96781 galactic UMa Second-epoch detections are separated by 0.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:43:31.50 +69:08:03.6 (user input) | T | P | (position from user input) J-Ks=0.581+/-0.028 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:43:31.50 +69:08:03.6: 14.01 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:43:31.50 +69:08:03.6: 14.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 43 31.50 +69 08 03.6 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.04,0.05,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
target 20260915.3628 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 13.04 10:08:36.54 +70:15:28.1
139.92446 41.07706 galactic UMa Second-epoch detections are separated by 0.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:08:36.54 +70:15:28.1 (user input) | T | P | (position from user input) J-Ks=0.415+/-0.030 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:08:36.54 +70:15:28.1: 14.04 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:08:36.54 +70:15:28.1: 14.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 10 08 36.54 +70 15 28.1 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.04,0.05,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
target 20260915.3628 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 13.01 09:14:11.92 +68:23:26.7
145.22721 37.96295 galactic UMa Second-epoch detections are separated by 1.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:14:11.92 +68:23:26.7 (user input) | T | P | (position from user input) J-Ks=0.451+/-0.037 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:14:11.92 +68:23:26.7: 14.03 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:14:11.92 +68:23:26.7: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 14 11.92 +68 23 26.7 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.01,0.05,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 20260915.3628 13.01CV 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 09 15.3628 2461298.8629 13.13 09:49:40.64 +69:26:21.9
142.07369 40.25934 galactic UMa Second-epoch detections are separated by 0.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:49:40.64 +69:26:21.9 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.033 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:49:40.64 +69:26:21.9: 14.19 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:49:40.64 +69:26:21.9: 14.16 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 49 40.64 +69 26 21.9 13.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.13,0.05,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
target 20260915.3628 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 12.76 10:37:48.79 +71:56:03.4
136.12960 41.59795 galactic UMa Second-epoch detections are separated by 1.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:37:48.79 +71:56:03.4 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.036 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:37:48.79 +71:56:03.4: 13.70 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:37:48.79 +71:56:03.4: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 10 37 48.79 +71 56 03.4 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.76,0.05,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 20260915.3628 12.76CV 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 09 15.3628 2461298.8629 12.80 09:20:28.13 +68:16:51.4
145.05120 38.53549 galactic UMa Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:20:28.13 +68:16:51.4 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.033 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:20:28.13 +68:16:51.4: 13.77 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:20:28.13 +68:16:51.4: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 20 28.13 +68 16 51.4 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.80,0.05,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 20260915.3628 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 12.81 09:21:29.83 +68:26:22.8
144.81593 38.55340 galactic UMa Second-epoch detections are separated by 1.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:21:29.83 +68:26:22.8 (user input) | T | P | (position from user input) J-Ks=0.365+/-0.059 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:21:29.83 +68:26:22.8: 13.75 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:21:29.83 +68:26:22.8: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 21 29.83 +68 26 22.8 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260915.3628 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 12.74 09:15:54.48 +67:26:26.0
146.25589 38.48797 galactic UMa Second-epoch detections are separated by 0.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:15:54.48 +67:26:26.0 (user input) | T | P | (position from user input) J-Ks=0.662+/-0.032 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:15:54.48 +67:26:26.0: 13.74 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:15:54.48 +67:26:26.0: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 15 54.48 +67 26 26.0 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.74,0.05,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 20260915.3628 12.74CV 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 09 15.3628 2461298.8629 12.69 09:26:01.17 +68:27:28.6
144.56074 38.91834 galactic UMa Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:26:01.17 +68:27:28.6 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.030 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:26:01.17 +68:27:28.6: 13.68 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:26:01.17 +68:27:28.6: 13.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.65 +/- 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 09 15.3628* 09 26 01.17 +68 27 28.6 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260915.3628 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 12.76 10:32:14.30 +72:44:05.3
135.84566 40.71823 galactic UMa Second-epoch detections are separated by 1.9" and 5.5 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 | 10:32:14.30 +72:44:05.3 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.033 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:32:14.30 +72:44:05.3: 13.67 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:32:14.30 +72:44:05.3: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 10 32 14.30 +72 44 05.3 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.76,0.05,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 20260915.3628 12.76CV 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 09 15.3628 2461298.8629 12.72 09:25:39.10 +68:42:41.2
144.28945 38.77430 galactic UMa Second-epoch detections are separated by 1.5" and 6.2 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 | Large-amplitude variable Gaia DR2 1069523100963624064 | 09:25:39.10 +68:42:41.2 (user input) | 2021A&A...648A..44M | | (position from user input) (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=0.703+/-0.030 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:25:39.10 +68:42:41.2: 13.67 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:25:39.10 +68:42:41.2: 13.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.66 +/- 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 09 15.3628* 09 25 39.10 +68 42 41.2 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1069523100963624064,2461298.8629,12.72,0.05,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 1069523100963624064 20260915.3628 12.72CV 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 09 15.3628 2461298.8629 12.68 10:31:12.34 +73:30:02.2
135.24575 40.09901 galactic Dra Second-epoch detections are separated by 0.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:31:12.34 +73:30:02.2 (user input) | T | P | (position from user input) J-Ks=0.457+/-0.028 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:31:12.34 +73:30:02.2: 13.62 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:31:12.34 +73:30:02.2: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.68,0.05,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 20260915.3628 12.68CV 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 09 15.3628 2461298.8629 12.65 09:28:21.94 +68:55:53.8
143.89419 38.89156 galactic UMa Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:28:21.94 +68:55:53.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:28:21.94 +68:55:53.8: 13.60 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:28:21.94 +68:55:53.8: 13.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 09 15.3628* 09 28 21.94 +68 55 53.8 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.65,0.05,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
target 20260915.3628 12.65CV 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 09 15.3628 2461298.8629 12.63 09:19:11.27 +67:53:36.9
145.56503 38.58941 galactic UMa Second-epoch detections are separated by 1.3" and 6.4 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 | Large-amplitude variable Gaia DR2 1069378210241893248 | 09:19:11.27 +67:53:36.9 (user input) | 2021A&A...648A..44M | | (position from user input) (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=0.821+/-0.030 (M)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:19:11.27 +67:53:36.9: 13.57 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:19:11.27 +67:53:36.9: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 19 11.27 +67 53 36.9 12.6 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
Large-amplitude variable Gaia DR2 1069378210241893248,2461298.8629,12.63,0.05,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 1069378210241893248 20260915.3628 12.63CV 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 09 15.3628 2461298.8629 12.62 09:38:27.78 +68:43:33.7
143.55628 39.78878 galactic UMa Second-epoch detections are separated by 1.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:38:27.78 +68:43:33.7 (user input) | T | P | (position from user input) J-Ks=0.438+/-0.032 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:38:27.78 +68:43:33.7: 13.58 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:38:27.78 +68:43:33.7: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.56 +/- 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 09 15.3628* 09 38 27.78 +68 43 33.7 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.62,0.05,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 20260915.3628 12.62CV 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 09 15.3628 2461298.8629 13.12 09:35:48.66 +70:33:06.6
141.67699 38.66291 galactic UMa Second-epoch detections are separated by 2.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:35:48.66 +70:33:06.6 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.030 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:35:48.66 +70:33:06.6: 14.30 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:35:48.66 +70:33:06.6: 14.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 35 48.66 +70 33 06.6 13.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.12,0.05,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
target 20260915.3628 13.12CV 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 09 15.3628 2461298.8629 13.03 09:35:17.38 +69:33:29.1
142.80739 39.12715 galactic UMa Second-epoch detections are separated by 0.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:35:17.38 +69:33:29.1 (user input) | T | P | (position from user input) J-Ks=0.532+/-0.028 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:35:17.38 +69:33:29.1: 14.23 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:35:17.38 +69:33:29.1: 14.04 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 35 17.38 +69 33 29.1 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.03,0.05,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 20260915.3628 13.03CV 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 09 15.3628 2461298.8629 13.07 09:59:21.55 +69:44:07.7
141.11487 40.77792 galactic UMa Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:59:21.55 +69:44:07.7 (user input) | T | P | (position from user input) J-Ks=0.529+/-0.034 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:59:21.55 +69:44:07.7: 14.21 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:59:21.55 +69:44:07.7: 14.20 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 59 21.55 +69 44 07.7 13.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.07,0.05,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
target 20260915.3628 13.07CV 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 09 15.3628 2461298.8629 12.99 10:26:26.62 +73:16:57.3
135.76573 40.02865 galactic Dra Second-epoch detections are separated by 3.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:26:26.62 +73:16:57.3 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.035 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:26:26.62 +73:16:57.3: 14.15 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:26:26.62 +73:16:57.3: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.99,0.05,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
target 20260915.3628 12.99CV 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 09 15.3628 2461298.8629 13.13 09:35:10.58 +68:22:38.9
144.14355 39.70017 galactic UMa Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:35:10.58 +68:22:38.9 (user input) | T | P | (position from user input) J-Ks=0.426+/-0.031 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:35:10.58 +68:22:38.9: 14.11 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:35:10.58 +68:22:38.9: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 35 10.58 +68 22 38.9 13.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.13,0.05,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
target 20260915.3628 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 13.05 09:31:25.96 +68:25:19.2
144.30673 39.37636 galactic UMa Second-epoch detections are separated by 3.6" and 5.7 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 | 09:31:25.96 +68:25:19.2 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.033 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:31:25.96 +68:25:19.2: 14.11 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:31:25.96 +68:25:19.2: 14.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 31 25.96 +68 25 19.2 13.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.05,0.05,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 20260915.3628 13.05CV 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 09 15.3628 2461298.8629 13.04 09:19:46.04 +68:07:36.8
145.26489 38.54144 galactic UMa Second-epoch detections are separated by 1.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:19:46.04 +68:07:36.8 (user input) | T | P | (position from user input) J-Ks=0.586+/-0.031 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:19:46.04 +68:07:36.8: 14.10 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:19:46.04 +68:07:36.8: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.04 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 19 46.04 +68 07 36.8 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.04,0.05,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
target 20260915.3628 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 12.90 09:41:07.10 +68:01:25.0
144.18703 40.35469 galactic UMa Second-epoch detections are separated by 3.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:41:07.10 +68:01:25.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:41:07.10 +68:01:25.0: 14.05 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:41:07.10 +68:01:25.0: 14.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 41 07.10 +68 01 25.0 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.90,0.05,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
target 20260915.3628 12.90CV 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 09 15.3628 2461298.8629 12.94 09:24:10.59 +68:10:17.5
144.98766 38.89289 galactic UMa Second-epoch detections are separated by 1.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:24:10.59 +68:10:17.5 (user input) | T | P | (position from user input) J-Ks=0.469+/-0.029 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:24:10.59 +68:10:17.5: 14.02 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:24:10.59 +68:10:17.5: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 24 10.59 +68 10 17.5 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.94,0.05,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 20260915.3628 12.94CV 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 09 15.3628 2461298.8629 13.02 09:15:23.55 +68:58:29.6
144.49475 37.82551 galactic UMa Second-epoch detections are separated by 2.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:15:23.55 +68:58:29.6 (user input) | T | P | (position from user input) J-Ks=0.757+/-0.033 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:15:23.55 +68:58:29.6: 13.99 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:15:23.55 +68:58:29.6: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 15 23.55 +68 58 29.6 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.02,0.05,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 20260915.3628 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 13.01 09:26:48.82 +69:05:43.5
143.79015 38.69265 galactic UMa Second-epoch detections are separated by 1.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:26:48.82 +69:05:43.5 (user input) | T | P | (position from user input) J-Ks=0.344+/-0.031 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:26:48.82 +69:05:43.5: 14.03 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:26:48.82 +69:05:43.5: 13.94 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 26 48.82 +69 05 43.5 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.01,0.05,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 20260915.3628 13.01CV 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 09 15.3628 2461298.8629 12.99 09:51:38.39 +69:28:28.4
141.90897 40.38224 galactic UMa Second-epoch detections are separated by 1.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:51:38.39 +69:28:28.4 (user input) | T | P | (position from user input) J-Ks=0.497+/-0.031 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:51:38.39 +69:28:28.4: 13.98 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:51:38.39 +69:28:28.4: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 51 38.39 +69 28 28.4 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.99,0.05,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
target 20260915.3628 12.99CV 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 09 15.3628 2461298.8629 13.04 09:25:01.27 +68:55:21.8
144.08063 38.62827 galactic UMa Second-epoch detections are separated by 3.5" and 6.9 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 | 09:25:01.27 +68:55:21.8 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.030 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:25:01.27 +68:55:21.8: 13.98 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:25:01.27 +68:55:21.8: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 25 01.27 +68 55 21.8 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.04,0.05,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
target 20260915.3628 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 12.98 09:16:38.85 +67:52:01.8
145.72076 38.38199 galactic UMa Second-epoch detections are separated by 1.7" and 6.7 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 | 09:16:38.85 +67:52:01.8 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.032 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:16:38.85 +67:52:01.8: 13.95 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:16:38.85 +67:52:01.8: 14.10 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 16 38.85 +67 52 01.8 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.98,0.05,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
target 20260915.3628 12.98CV 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 09 15.3628 2461298.8629 12.97 10:11:42.07 +70:18:29.2
139.65021 41.24415 galactic UMa Second-epoch detections are separated by 1.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:42.07 +70:18:29.2 (user input) | T | P | (position from user input) J-Ks=0.474+/-0.033 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:11:42.07 +70:18:29.2: 13.95 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:11:42.07 +70:18:29.2: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 10 11 42.07 +70 18 29.2 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.97,0.05,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
target 20260915.3628 12.97CV 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 09 15.3628 2461298.8629 13.01 09:38:15.28 +70:34:48.6
141.51115 38.82224 galactic UMa Second-epoch detections are separated by 1.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:38:15.28 +70:34:48.6 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.029 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:38:15.28 +70:34:48.6: 13.91 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:38:15.28 +70:34:48.6: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 38 15.28 +70 34 48.6 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.01,0.05,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 20260915.3628 13.01CV 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 09 15.3628 2461298.8629 12.89 09:23:40.79 +68:51:26.7
144.22445 38.54945 galactic UMa Second-epoch detections are separated by 1.8" and 6.6 pix
The object was found in VSX 1" ZTF J092340.86+685126.2
Type: DSCT
# Max. Min./Amp. JD0 Period
13.921 g Y 0.123 g 2458210.75170 0.065015400000
The object was not found in astcheck.
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:23:40.79 +68:51:26.7: 13.89 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:23:40.79 +68:51:26.7: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 23 40.79 +68 51 26.7 12.9 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
ZTF J092340.86+685126.2,2461298.8629,12.89,0.05,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
ZTF J092340.86+685126.2 20260915.3628 12.89CV 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
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 13.02 09:34:53.61 +67:26:17.7
145.23423 40.12799 galactic UMa Second-epoch detections are separated by 2.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:34:53.61 +67:26:17.7 (user input) | T | P | (position from user input) J-Ks=0.483+/-0.028 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:34:53.61 +67:26:17.7: 13.91 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:34:53.61 +67:26:17.7: 13.96 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 34 53.61 +67 26 17.7 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.02,0.05,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 20260915.3628 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 13.03 09:50:25.92 +68:59:15.1
142.51834 40.56605 galactic UMa Second-epoch detections are separated by 1.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:50:25.92 +68:59:15.1 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.032 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:50:25.92 +68:59:15.1: 13.92 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:50:25.92 +68:59:15.1: 13.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 50 25.92 +68 59 15.1 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,13.03,0.05,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 20260915.3628 13.03CV 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 09 15.3628 2461298.8629 12.97 09:18:42.19 +68:06:24.5
145.34107 38.45970 galactic UMa Second-epoch detections are separated by 1.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:18:42.19 +68:06:24.5 (user input) | T | P | (position from user input) J-Ks=0.315+/-0.032 (F)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:18:42.19 +68:06:24.5: 13.94 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:18:42.19 +68:06:24.5: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 18 42.19 +68 06 24.5 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.97,0.05,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
target 20260915.3628 12.97CV 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 09 15.3628 2461298.8629 12.88 09:48:33.28 +69:08:54.5
142.46353 40.33740 galactic UMa Second-epoch detections are separated by 1.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:48:33.28 +69:08:54.5 (user input) | T | P | (position from user input) J-Ks=0.519+/-0.030 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:48:33.28 +69:08:54.5: 13.88 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:48:33.28 +69:08:54.5: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 48 33.28 +69 08 54.5 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260915.3628 12.88CV 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 09 15.3628 2461298.8629 12.88 09:01:00.51 +66:53:49.0
147.55972 37.33666 galactic UMa Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:01:00.51 +66:53:49.0 (user input) | T | P | (position from user input) J-Ks=0.328+/-0.036 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:01:00.51 +66:53:49.0: 13.87 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:01:00.51 +66:53:49.0: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 01 00.51 +66 53 49.0 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260915.3628 12.88CV 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 09 15.3628 2461298.8629 12.89 09:34:30.35 +68:23:33.0
144.16537 39.63888 galactic UMa Second-epoch detections are separated by 1.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:34:30.35 +68:23:33.0 (user input) | T | P | (position from user input) J-Ks=0.485+/-0.028 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:34:30.35 +68:23:33.0: 13.88 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:34:30.35 +68:23:33.0: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 34 30.35 +68 23 33.0 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.89,0.05,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
target 20260915.3628 12.89CV 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
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 12.91 09:33:38.33 +68:29:53.8
144.09500 39.51810 galactic UMa Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:33:38.33 +68:29:53.8 (user input) | T | P | (position from user input) J-Ks=0.367+/-0.028 (G)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:33:38.33 +68:29:53.8: 13.85 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:33:38.33 +68:29:53.8: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 33 38.33 +68 29 53.8 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.91,0.05,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 20260915.3628 12.91CV 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 09 15.3628 2461298.8629 12.82 09:29:00.64 +69:19:07.4
143.42048 38.76130 galactic UMa Second-epoch detections are separated by 1.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:29:00.64 +69:19:07.4 (user input) | T | P | (position from user input) J-Ks=0.708+/-0.027 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:29:00.64 +69:19:07.4: 13.82 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:29:00.64 +69:19:07.4: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 29 00.64 +69 19 07.4 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.82,0.05,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 20260915.3628 12.82CV 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 09 15.3628 2461298.8629 12.96 09:24:05.08 +68:11:42.6
144.96517 38.87486 galactic UMa Second-epoch detections are separated by 1.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:24:05.08 +68:11:42.6 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.033 (F)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:24:05.08 +68:11:42.6: 13.84 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:24:05.08 +68:11:42.6: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 24 05.08 +68 11 42.6 13.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.96,0.05,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
target 20260915.3628 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 15.3628 2461298.8629 12.88 09:16:28.46 +68:06:51.0
145.44119 38.26723 galactic UMa Second-epoch detections are separated by 2.5" and 6.7 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 | 09:16:28.46 +68:06:51.0 (user input) | T | P | (position from user input) J-Ks=0.628+/-0.036 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:16:28.46 +68:06:51.0: 13.78 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:16:28.46 +68:06:51.0: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 16 28.46 +68 06 51.0 12.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260915.3628 12.88CV 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 09 15.3628 2461298.8629 12.85 09:33:30.84 +70:35:10.7
141.76301 38.48081 galactic UMa Second-epoch detections are separated by 1.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:33:30.84 +70:35:10.7 (user input) | T | P | (position from user input) J-Ks=0.649+/-0.028 (K)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:33:30.84 +70:35:10.7: 13.78 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:33:30.84 +70:35:10.7: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 15.3628* 09 33 30.84 +70 35 10.7 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461298.8629,12.85,0.05,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 20260915.3628 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79736027 11.02.2026 07:08:01.927 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
First image: 2461082.79736027 11.02.2026 07:08:01.927 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Last image: 2461298.86316063 15.09.2026 08:42:47.078 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 2 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 8464
Objects passed selection criteria: 8430
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 5784.5
Average stars matched: 5615.5 (97.0784 %)
Memory usage VmPeak: 234536 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 15 03:45:13 CDT 2026
Host name: tau
############################################################
ERROR: large change in astrometric-star counts between the two new images (q3: 559 -> 437, 21.825% > 20%; fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits vs fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits) - possible passing clouds or a bad plate solution; continuing processing
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.79736027 11.02.2026 07:08:01.927 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
First image: 2461082.79736027 11.02.2026 07:08:01.927 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Last image: 2461298.86316063 15.09.2026 08:42:47.078 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 61
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.14
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 10 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 48390
Objects passed selection criteria: 48241
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 34313.2
Average stars matched: 33085.8 (96.4227 %)
Memory usage VmPeak: 269968 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 15 03:45:52 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
SExtractor catalog cache: saved UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.cat to cache
SExtractor catalog cache: saved UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.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: 2461298.86253920
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits exists and is non-empty
wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits exists and is non-empty
wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits exists and is non-empty
wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits (1st reference image)
verification OK: wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Image size: 941.6'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:36:20.346 +69:59:16.26 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits (1st new image)
verification OK: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
Image size: 942.3'x626.8' 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: 09:36:55.516 +70:01:02.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:36:20.346 +69:59:16.26
Second-epoch image center 09:36:55.516 +70:01:02.73
Angular distance between the image centers 0.0582 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits (2nd new image)
verification OK: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
Image size: 942.3'x626.8' 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: 09:36:58.682 +70:00:29.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:36:20.346 +69:59:16.26
Second-epoch image center 09:36:58.682 +70:00:29.73
Angular distance between the image centers 0.0583 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:36:55.516 +70:01:02.73
Second-epoch second image center 09:36:58.682 +70:00:29.73
Angular distance between the image centers 0.01022 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits &> /tmp/tmp.umu9A0dLAu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits &> /tmp/tmp.D93vhsdARz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits &> /tmp/tmp.64q9ej9KCJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits &> /tmp/tmp.VSxAspgvhb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits and wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits and wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
Found non-empty wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits and wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
The reference image (wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits) and catalog (wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat) found
'wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat' -> 'wcsmag.cat'
Read 8779 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 117.0324 to 171.9972 deg, Dec +62.9079 to +75.4793 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 117.0324 to 171.9972 deg, Dec 62.9079 to 75.4793 deg
Loaded 9306 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): 5117 out of 5413 total matches.
Matched with Tycho-2 5413 out of 8779 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.870000
a=0.000000 b=1.000000 c=22.870000
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8779 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 117.0324 to 171.9972 deg, Dec +62.9079 to +75.4793 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 117.0324 to 171.9972 deg, Dec 62.9079 to 75.4793 deg
Loaded 9306 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): 5117 out of 5413 total matches.
Matched with Tycho-2 5413 out of 8779 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Forced-photometry filter: calibrated wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits -> calib.txt_param_ref_wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits (aperture=6.1)
Read 8894 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 117.0326 to 171.9963 deg, Dec +62.9079 to +75.4793 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 117.0326 to 171.9963 deg, Dec 62.9079 to 75.4793 deg
Loaded 9306 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): 5133 out of 5416 total matches.
Matched with Tycho-2 5416 out of 8894 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Forced-photometry filter: calibrated wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits -> calib.txt_param_ref_wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
2.1 pix UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
2.4 pix fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
2.4 pix fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
Limiting magnitude estimates:
15.5 mag. UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
15.5 mag. UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
13.3 mag. fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
13.2 mag. fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.umu9A0dLAu (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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits' -> 'wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WCS_IMAGE_NAME=wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WCS-calibrated image found: wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Checking if the catalog wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits alredy exist and is non-empty...
Catalog wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WCS catalog name: wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=680, bad_region=0, passed=8779
Got 8779 stars (including 8092 good ones) from the SExtractor catalog wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
util/solve_plate_with_UCAC5 got 8779 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 4890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 4886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 8779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 4890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 8779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 8779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4886 stars left (next iteration limit 5374)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits N_match=4886 sigma_overall_arcsec=0.367 sigma_q1_arcsec=0.507 sigma_q2_arcsec=0.349 sigma_q3_arcsec=0.377 sigma_q4_arcsec=0.300 n_q1=1067 n_q2=1443 n_q3=1095 n_q4=1281 worst_quadrant_to_overall_ratio=1.381
The image catalog is written to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits -region wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.D93vhsdARz (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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits' -> 'wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WCS_IMAGE_NAME=wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WCS-calibrated image found: wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Checking if the catalog wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat corresponding to the image wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits alredy exist and is non-empty...
Catalog wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat corresponding to the image wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WCS catalog name: wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=664, bad_region=0, passed=8894
Got 8894 stars (including 8220 good ones) from the SExtractor catalog wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat
util/solve_plate_with_UCAC5 got 8894 stars from the SExtractor catalog
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 4886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 8894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 8894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 8894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4886 stars left (next iteration limit 5374)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits N_match=4886 sigma_overall_arcsec=0.368 sigma_q1_arcsec=0.498 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.363 sigma_q4_arcsec=0.309 n_q1=1066 n_q2=1431 n_q3=1117 n_q4=1272 worst_quadrant_to_overall_ratio=1.353
The image catalog is written to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits -region wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.64q9ej9KCJ (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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
WCS_IMAGE_NAME=wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
WCS-calibrated image found: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
Checking if the catalog wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
WCS catalog name: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=133, bad_region=0, passed=2874
Got 2874 stars (including 2740 good ones) from the SExtractor catalog wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat
util/solve_plate_with_UCAC5 got 2874 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 2664 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2660 matched stars entering correct_measured_positions(), 2661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2660 matched stars entering correct_measured_positions(), 2873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 2663 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2659 matched stars entering correct_measured_positions(), 2872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 2659 matched stars entering correct_measured_positions(), 2872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 2659 stars left (next iteration limit 2926)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2659 robust_rms=10.429 arcsec worst_quadrant_rms=12.633 arcsec
SIP_REFIT: SIP order 3 trial: matched=2659 robust_rms=0.609 arcsec worst_quadrant_rms=0.705 arcsec
SIP_REFIT: SIP order 5 trial: matched=2659 robust_rms=0.443 arcsec worst_quadrant_rms=0.555 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2659 robust_rms_before=1.100 arcsec robust_rms_before_corrected=0.374 arcsec robust_rms_after=0.443 arcsec worst_quadrant_rms_before=0.430 worst_quadrant_rms_after=0.555
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.430 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits N_match=2659 sigma_overall_arcsec=0.395 sigma_q1_arcsec=0.370 sigma_q2_arcsec=0.451 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.408 n_q1=778 n_q2=644 n_q3=559 n_q4=678 worst_quadrant_to_overall_ratio=1.142
The image catalog is written to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits -region wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.VSxAspgvhb (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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
WCS_IMAGE_NAME=wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
WCS-calibrated image found: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
Checking if the catalog wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
WCS catalog name: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=126, bad_region=0, passed=2721
Got 2721 stars (including 2587 good ones) from the SExtractor catalog wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat
util/solve_plate_with_UCAC5 got 2721 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 2517 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2513 matched stars entering correct_measured_positions(), 2513 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2513 matched stars entering correct_measured_positions(), 2720 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 767 to 828 (Dec 63.6 to 75.3)
Done reading UCAC5 zone files...
Matched 2517 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2513 matched stars entering correct_measured_positions(), 2720 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 2513 matched stars entering correct_measured_positions(), 2720 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 2513 stars left (next iteration limit 2764)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2513 robust_rms=9.596 arcsec worst_quadrant_rms=11.162 arcsec
SIP_REFIT: SIP order 3 trial: matched=2513 robust_rms=0.601 arcsec worst_quadrant_rms=0.666 arcsec
SIP_REFIT: SIP order 5 trial: matched=2513 robust_rms=0.436 arcsec worst_quadrant_rms=0.487 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2513 robust_rms_before=1.089 arcsec robust_rms_before_corrected=0.391 arcsec robust_rms_after=0.436 arcsec worst_quadrant_rms_before=0.441 worst_quadrant_rms_after=0.487
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.441 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits N_match=2513 sigma_overall_arcsec=0.394 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.468 sigma_q3_arcsec=0.384 sigma_q4_arcsec=0.383 n_q1=737 n_q2=658 n_q3=437 n_q4=681 worst_quadrant_to_overall_ratio=1.188
The image catalog is written to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits -region wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits to local_wcs_cache/
'wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits' -> 'local_wcs_cache/wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits'
Saving the final (post-refit) wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits to local_wcs_cache/
'wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits' -> 'local_wcs_cache/wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits'
Saving the final (post-refit) wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits to local_wcs_cache/
'wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits' -> 'local_wcs_cache/wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits'
Saving the final (post-refit) wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits to local_wcs_cache/
'wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits' -> 'local_wcs_cache/wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits sigma_overall=0.367 worst_q_ratio=1.381
ref2=UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits sigma_overall=0.368 worst_q_ratio=1.353
new1=fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits sigma_overall=0.395 worst_q_ratio=1.142
new2=fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits sigma_overall=0.394 worst_q_ratio=1.188
reference average sigma_overall=0.3675 worst_q_ratio=1.367
warn-on-ratio threshold: 2.0x reference
###################################
ERROR: large change in astrometric-star counts between the two new images (q3: 559 -> 437, 21.825% > 20%; fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits vs fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits) - possible passing clouds or a bad plate solution; continuing processing
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292_astrometric_residuals.png (4886 matched stars from wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293_astrometric_residuals.png (4886 matched stars from wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325_astrometric_residuals.png (2659 matched stars from wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326_astrometric_residuals.png (2513 matched stars from wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits'
Saving fully-calibrated image wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits'
Preparing the HTML report for the field UMa-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field UMa-01-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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
SExtractor catalog cache: saved UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.cat to cache
SExtractor catalog cache: saved UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Creating symlink local_wcs_cache/wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits exists and is non-empty
wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits exists and is non-empty
wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits exists and is non-empty
wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits (1st reference image)
verification OK: wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Image size: 941.6'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:36:20.346 +69:59:16.26 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits (1st new image)
verification OK: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
Image size: 942.3'x626.8' 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: 09:36:55.516 +70:01:02.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:36:20.346 +69:59:16.26
Second-epoch image center 09:36:55.516 +70:01:02.73
Angular distance between the image centers 0.0582 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits (2nd new image)
verification OK: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
Image size: 942.3'x626.8' 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: 09:36:58.682 +70:00:29.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:36:20.346 +69:59:16.26
Second-epoch image center 09:36:58.682 +70:00:29.73
Angular distance between the image centers 0.0583 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:36:55.516 +70:01:02.73
Second-epoch second image center 09:36:58.682 +70:00:29.73
Angular distance between the image centers 0.01022 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits &> /tmp/tmp.fwur9c7EcX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits &> /tmp/tmp.OhslslrUki
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits &> /tmp/tmp.6q3CECOY9g
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits &> /tmp/tmp.Idi5seXEG7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits and wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits and wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
Found non-empty wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits and wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
The reference image (wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits) and catalog (wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat) found
'wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat' -> 'wcsmag.cat'
Read 51532 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 116.7731 to 172.6868 deg, Dec +62.8119 to +75.4848 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 116.7731 to 172.6868 deg, Dec 62.8119 to 75.4848 deg
Loaded 9545 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4865 out of 5490 total matches.
Matched with Tycho-2 5490 out of 51532 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.754400
a=0.000000 b=1.000000 c=22.754400
From vast_summary.log: estimated ref. image limiting mag.: -7.14
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 51532 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 116.7731 to 172.6868 deg, Dec +62.8119 to +75.4848 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 116.7731 to 172.6868 deg, Dec 62.8119 to 75.4848 deg
Loaded 9545 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4865 out of 5490 total matches.
Matched with Tycho-2 5490 out of 51532 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Forced-photometry filter: calibrated wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits -> calib.txt_param_ref_wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits (aperture=4.7)
Read 51887 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 116.6991 to 172.5281 deg, Dec +62.8124 to +75.4915 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 116.6991 to 172.5281 deg, Dec 62.8124 to 75.4915 deg
Loaded 9544 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4853 out of 5491 total matches.
Matched with Tycho-2 5491 out of 51887 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Forced-photometry filter: calibrated wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits -> calib.txt_param_ref_wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 60 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
1.9 pix UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
2.3 pix fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
2.3 pix fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
Limiting magnitude estimates:
15.6 mag. UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
15.6 mag. UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
13.5 mag. fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
13.5 mag. fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 13.2 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.fwur9c7EcX (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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits' -> 'wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WCS_IMAGE_NAME=wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WCS-calibrated image found: wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
Checking if the catalog wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits alredy exist and is non-empty...
Catalog wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits
WCS catalog name: wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2624, bad_region=3, passed=51519
Got 51519 stars (including 48797 good ones) from the SExtractor catalog wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat
util/solve_plate_with_UCAC5 got 51519 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 4894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 51519 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 51519 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 51519 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4894 stars left (next iteration limit 5383)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits N_match=4894 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.496 sigma_q2_arcsec=0.330 sigma_q3_arcsec=0.350 sigma_q4_arcsec=0.286 n_q1=1073 n_q2=1412 n_q3=1115 n_q4=1294 worst_quadrant_to_overall_ratio=1.422
The image catalog is written to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits -region wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.OhslslrUki (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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits' -> 'wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WCS_IMAGE_NAME=wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WCS-calibrated image found: wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
Checking if the catalog wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat corresponding to the image wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits alredy exist and is non-empty...
Catalog wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat corresponding to the image wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits
WCS catalog name: wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=2687, bad_region=5, passed=51863
Got 51863 stars (including 49074 good ones) from the SExtractor catalog wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat
util/solve_plate_with_UCAC5 got 51863 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 4896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 51863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 51863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 51863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4896 stars left (next iteration limit 5385)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits N_match=4896 sigma_overall_arcsec=0.345 sigma_q1_arcsec=0.469 sigma_q2_arcsec=0.325 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.303 n_q1=1092 n_q2=1397 n_q3=1115 n_q4=1292 worst_quadrant_to_overall_ratio=1.361
The image catalog is written to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits -region wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.6q3CECOY9g (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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
WCS_IMAGE_NAME=wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
WCS-calibrated image found: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
Checking if the catalog wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
WCS catalog name: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=349, bad_region=14, passed=17862
Got 17862 stars (including 17485 good ones) from the SExtractor catalog wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat
util/solve_plate_with_UCAC5 got 17862 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.4 to 75.3)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 4863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 17862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.4 to 75.3)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 17862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 17862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4863 stars left (next iteration limit 5349)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4863 robust_rms=9.383 arcsec worst_quadrant_rms=14.129 arcsec
SIP_REFIT: SIP order 3 trial: matched=4863 robust_rms=0.633 arcsec worst_quadrant_rms=0.725 arcsec
SIP_REFIT: SIP order 5 trial: matched=4863 robust_rms=0.472 arcsec worst_quadrant_rms=0.576 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4863 robust_rms_before=1.110 arcsec robust_rms_before_corrected=0.404 arcsec robust_rms_after=0.472 arcsec worst_quadrant_rms_before=0.463 worst_quadrant_rms_after=0.576
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.463 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits N_match=4863 sigma_overall_arcsec=0.406 sigma_q1_arcsec=0.390 sigma_q2_arcsec=0.463 sigma_q3_arcsec=0.384 sigma_q4_arcsec=0.402 n_q1=1442 n_q2=1124 n_q3=1107 n_q4=1190 worst_quadrant_to_overall_ratio=1.140
The image catalog is written to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits -region wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Idi5seXEG7 (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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
WCS_IMAGE_NAME=wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
WCS-calibrated image found: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
Checking if the catalog wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat corresponding to the image wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
WCS catalog name: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=356, bad_region=19, passed=16932
Got 16932 stars (including 16522 good ones) from the SExtractor catalog wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat
util/solve_plate_with_UCAC5 got 16932 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.4 to 75.3)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 4865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 16932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 766 to 828 (Dec 63.4 to 75.3)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 16932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 16932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4864 stars left (next iteration limit 5351)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4864 robust_rms=9.479 arcsec worst_quadrant_rms=11.825 arcsec
SIP_REFIT: SIP order 3 trial: matched=4864 robust_rms=0.641 arcsec worst_quadrant_rms=0.675 arcsec
SIP_REFIT: SIP order 5 trial: matched=4864 robust_rms=0.483 arcsec worst_quadrant_rms=0.539 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4864 robust_rms_before=1.107 arcsec robust_rms_before_corrected=0.429 arcsec robust_rms_after=0.483 arcsec worst_quadrant_rms_before=0.476 worst_quadrant_rms_after=0.539
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.476 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits N_match=4864 sigma_overall_arcsec=0.433 sigma_q1_arcsec=0.397 sigma_q2_arcsec=0.486 sigma_q3_arcsec=0.427 sigma_q4_arcsec=0.411 n_q1=1429 n_q2=1207 n_q3=947 n_q4=1281 worst_quadrant_to_overall_ratio=1.123
The image catalog is written to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits -region wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-41-53_20.00sec_-0.00C_LIGHTs_0325.fits
Saving fully-calibrated image wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.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_2026-09-15_CI_UMa-01-Q1b1x1_034339_TTUQ1b1x1_4006135_k91nbsNy/wcs_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326.fits
Preparing the HTML report for the field UMa-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 08:59:19.05 +67:23:45.5: 13.18 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:18:43.24 +67:14:21.5: 13.04 +/- 0.02 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 11:15:05.28 +72:01:05.7: 12.67 +/- 0.02 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:26:23.20 +67:35:20.9: 13.85 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:18:33.47 +68:41:51.1: 13.82 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:35:48.89 +74:00:32.5: 13.87 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:08:36.54 +70:15:28.1: 14.04 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:41:17.54 +69:40:53.4: 13.94 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:14:11.92 +68:23:26.7: 14.03 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:43:31.50 +69:08:03.6: 14.01 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 08:59:19.05 +67:23:45.5: 13.14 +/- 0.02 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 11:15:05.28 +72:01:05.7: 12.64 +/- 0.02 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:18:43.24 +67:14:21.5: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter REJECTED candidate at 08:59:19.05 +67:23:45.5: ref_mag=13.16 +/- 0.02 new_mean_mag=12.8880 delta=0.27 (need > 0.90)
Forced photometry reference-image weighted average: 13.03 +/- 0.01
Forced photometry filter REJECTED candidate at 11:15:05.28 +72:01:05.7: ref_mag=12.66 +/- 0.01 new_mean_mag=12.3131 delta=0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:18:43.24 +67:14:21.5: ref_mag=13.03 +/- 0.01 new_mean_mag=12.5524 delta=0.47 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:26:23.20 +67:35:20.9: 13.84 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:18:33.47 +68:41:51.1: 13.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.03
Forced photometry filter KEPT candidate at 09:26:23.20 +67:35:20.9: ref_mag=13.84 +/- 0.03 new_mean_mag=12.9261 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Forced photometry filter KEPT candidate at 09:18:33.47 +68:41:51.1: ref_mag=13.85 +/- 0.03 new_mean_mag=12.9179 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:35:48.89 +74:00:32.5: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry filter KEPT candidate at 10:35:48.89 +74:00:32.5: ref_mag=13.94 +/- 0.04 new_mean_mag=12.8302 delta=1.11 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:41:17.54 +69:40:53.4: 13.91 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:43:31.50 +69:08:03.6: 14.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.03
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:14:11.92 +68:23:26.7: 13.98 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:08:36.54 +70:15:28.1: 14.22 +/- 0.06 detection
Forced photometry filter KEPT candidate at 09:41:17.54 +69:40:53.4: ref_mag=13.93 +/- 0.03 new_mean_mag=12.9199 delta=1.01 (need > 0.90)
Forced photometry reference-image weighted average: 14.01 +/- 0.03
Forced photometry reference-image weighted average: 14.01 +/- 0.03
Forced photometry reference-image weighted average: 14.11 +/- 0.04
Forced photometry filter KEPT candidate at 09:43:31.50 +69:08:03.6: ref_mag=14.01 +/- 0.03 new_mean_mag=13.0368 delta=0.97 (need > 0.90)
Forced photometry filter KEPT candidate at 09:14:11.92 +68:23:26.7: ref_mag=14.01 +/- 0.03 new_mean_mag=12.9976 delta=1.01 (need > 0.90)
Forced photometry filter KEPT candidate at 10:08:36.54 +70:15:28.1: ref_mag=14.11 +/- 0.04 new_mean_mag=13.0384 delta=1.07 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:49:40.64 +69:26:21.9: 14.19 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:37:48.79 +71:56:03.4: 13.70 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:20:28.13 +68:16:51.4: 13.77 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:49:40.64 +69:26:21.9: 14.16 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:37:48.79 +71:56:03.4: 13.71 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:20:28.13 +68:16:51.4: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.04
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry filter KEPT candidate at 09:49:40.64 +69:26:21.9: ref_mag=14.18 +/- 0.04 new_mean_mag=13.1261 delta=1.05 (need > 0.90)
Forced photometry filter KEPT candidate at 10:37:48.79 +71:56:03.4: ref_mag=13.70 +/- 0.03 new_mean_mag=12.7582 delta=0.94 (need > 0.90)
Forced photometry filter KEPT candidate at 09:20:28.13 +68:16:51.4: ref_mag=13.76 +/- 0.03 new_mean_mag=12.7990 delta=0.96 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:21:29.83 +68:26:22.8: 13.75 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:21:29.83 +68:26:22.8: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter KEPT candidate at 09:21:29.83 +68:26:22.8: ref_mag=13.73 +/- 0.03 new_mean_mag=12.8125 delta=0.91 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:26:01.17 +68:27:28.6: 13.68 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:15:54.48 +67:26:26.0: 13.74 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:32:14.30 +72:44:05.3: 13.67 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:25:39.10 +68:42:41.2: 13.67 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:31:12.34 +73:30:02.2: 13.62 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:28:21.94 +68:55:53.8: 13.60 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:19:11.27 +67:53:36.9: 13.57 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:26:01.17 +68:27:28.6: 13.63 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:15:54.48 +67:26:26.0: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.02
Forced photometry filter KEPT candidate at 09:26:01.17 +68:27:28.6: ref_mag=13.65 +/- 0.02 new_mean_mag=12.6896 delta=0.96 (need > 0.90)
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:32:14.30 +72:44:05.3: 13.68 +/- 0.04 detection
Forced photometry filter KEPT candidate at 09:15:54.48 +67:26:26.0: ref_mag=13.69 +/- 0.03 new_mean_mag=12.7416 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 10:32:14.30 +72:44:05.3: ref_mag=13.68 +/- 0.03 new_mean_mag=12.7518 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:25:39.10 +68:42:41.2: 13.65 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:31:12.34 +73:30:02.2: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.02
Forced photometry filter KEPT candidate at 09:25:39.10 +68:42:41.2: ref_mag=13.66 +/- 0.02 new_mean_mag=12.7187 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Forced photometry filter KEPT candidate at 10:31:12.34 +73:30:02.2: ref_mag=13.63 +/- 0.03 new_mean_mag=12.6805 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:28:21.94 +68:55:53.8: 13.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Forced photometry filter KEPT candidate at 09:28:21.94 +68:55:53.8: ref_mag=13.62 +/- 0.02 new_mean_mag=12.6483 delta=0.97 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:19:11.27 +67:53:36.9: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter KEPT candidate at 09:19:11.27 +67:53:36.9: ref_mag=13.59 +/- 0.03 new_mean_mag=12.6248 delta=0.96 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:38:27.78 +68:43:33.7: 13.58 +/- 0.03 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:38:27.78 +68:43:33.7: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.02
Forced photometry filter KEPT candidate at 09:38:27.78 +68:43:33.7: ref_mag=13.56 +/- 0.02 new_mean_mag=12.6240 delta=0.93 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:35:48.66 +70:33:06.6: 14.30 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:35:48.66 +70:33:06.6: 14.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.05
Forced photometry filter KEPT candidate at 09:35:48.66 +70:33:06.6: ref_mag=14.34 +/- 0.05 new_mean_mag=13.0741 delta=1.26 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:35:17.38 +69:33:29.1: 14.23 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:35:17.38 +69:33:29.1: 14.04 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.04
Forced photometry filter KEPT candidate at 09:35:17.38 +69:33:29.1: ref_mag=14.12 +/- 0.04 new_mean_mag=13.0177 delta=1.10 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:59:21.55 +69:44:07.7: 14.21 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:26:26.62 +73:16:57.3: 14.15 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:31:25.96 +68:25:19.2: 14.11 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:35:10.58 +68:22:38.9: 14.11 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:19:46.04 +68:07:36.8: 14.10 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:59:21.55 +69:44:07.7: 14.20 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:41:07.10 +68:01:25.0: 14.05 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.04
Forced photometry filter KEPT candidate at 09:59:21.55 +69:44:07.7: ref_mag=14.20 +/- 0.04 new_mean_mag=13.0381 delta=1.17 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:24:10.59 +68:10:17.5: 14.02 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:26:26.62 +73:16:57.3: 14.13 +/- 0.06 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:31:25.96 +68:25:19.2: 14.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.04
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:19:46.04 +68:07:36.8: 13.99 +/- 0.05 detection
Forced photometry filter KEPT candidate at 10:26:26.62 +73:16:57.3: ref_mag=14.14 +/- 0.04 new_mean_mag=12.9516 delta=1.19 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:35:10.58 +68:22:38.9: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Forced photometry reference-image weighted average: 14.04 +/- 0.04
Forced photometry filter KEPT candidate at 09:31:25.96 +68:25:19.2: ref_mag=14.10 +/- 0.04 new_mean_mag=13.0499 delta=1.05 (need > 0.90)
Forced photometry filter KEPT candidate at 09:19:46.04 +68:07:36.8: ref_mag=14.04 +/- 0.04 new_mean_mag=13.0337 delta=1.00 (need > 0.90)
Forced photometry reference-image weighted average: 14.11 +/- 0.04
Forced photometry filter KEPT candidate at 09:35:10.58 +68:22:38.9: ref_mag=14.11 +/- 0.04 new_mean_mag=13.1213 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:41:07.10 +68:01:25.0: 14.01 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.03
Forced photometry filter KEPT candidate at 09:41:07.10 +68:01:25.0: ref_mag=14.03 +/- 0.03 new_mean_mag=12.8914 delta=1.14 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:24:10.59 +68:10:17.5: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.04
Forced photometry filter KEPT candidate at 09:24:10.59 +68:10:17.5: ref_mag=14.01 +/- 0.04 new_mean_mag=12.9354 delta=1.07 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:15:23.55 +68:58:29.6: 13.99 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:15:23.55 +68:58:29.6: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.03
Forced photometry filter KEPT candidate at 09:15:23.55 +68:58:29.6: ref_mag=14.01 +/- 0.03 new_mean_mag=13.0043 delta=1.01 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:26:48.82 +69:05:43.5: 14.03 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:26:48.82 +69:05:43.5: 13.94 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.03
Forced photometry filter KEPT candidate at 09:26:48.82 +69:05:43.5: ref_mag=13.98 +/- 0.03 new_mean_mag=13.0060 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:51:38.39 +69:28:28.4: 13.98 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:51:38.39 +69:28:28.4: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.03
Forced photometry filter KEPT candidate at 09:51:38.39 +69:28:28.4: ref_mag=13.96 +/- 0.03 new_mean_mag=12.9854 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:25:01.27 +68:55:21.8: 13.98 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:16:38.85 +67:52:01.8: 13.95 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 10:11:42.07 +70:18:29.2: 13.95 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:38:15.28 +70:34:48.6: 13.91 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:23:40.79 +68:51:26.7: 13.89 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:25:01.27 +68:55:21.8: 14.03 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.03
Forced photometry filter KEPT candidate at 09:25:01.27 +68:55:21.8: ref_mag=14.00 +/- 0.03 new_mean_mag=12.9891 delta=1.02 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:34:53.61 +67:26:17.7: 13.91 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:16:38.85 +67:52:01.8: 14.10 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:50:25.92 +68:59:15.1: 13.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.03
Forced photometry filter KEPT candidate at 09:16:38.85 +67:52:01.8: ref_mag=14.02 +/- 0.03 new_mean_mag=12.9522 delta=1.06 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 10:11:42.07 +70:18:29.2: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.03
Forced photometry filter KEPT candidate at 10:11:42.07 +70:18:29.2: ref_mag=13.96 +/- 0.03 new_mean_mag=12.9685 delta=0.99 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:38:15.28 +70:34:48.6: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.03
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:23:40.79 +68:51:26.7: 13.90 +/- 0.05 detection
Forced photometry filter KEPT candidate at 09:38:15.28 +70:34:48.6: ref_mag=13.93 +/- 0.03 new_mean_mag=12.9840 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 13.90 +/- 0.03
Forced photometry filter KEPT candidate at 09:23:40.79 +68:51:26.7: ref_mag=13.90 +/- 0.03 new_mean_mag=12.8959 delta=1.00 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:34:53.61 +67:26:17.7: 13.96 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.03
Forced photometry filter KEPT candidate at 09:34:53.61 +67:26:17.7: ref_mag=13.94 +/- 0.03 new_mean_mag=12.9816 delta=0.95 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:50:25.92 +68:59:15.1: 13.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.03
Forced photometry filter KEPT candidate at 09:50:25.92 +68:59:15.1: ref_mag=13.92 +/- 0.03 new_mean_mag=13.0189 delta=0.90 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:27:37.76 +67:44:43.9: 13.79 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:27:37.76 +67:44:43.9: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter REJECTED candidate at 09:27:37.76 +67:44:43.9: ref_mag=13.77 +/- 0.03 new_mean_mag=12.9286 delta=0.84 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:18:42.19 +68:06:24.5: 13.94 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:36:23.83 +68:50:09.1: 13.88 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:48:33.28 +69:08:54.5: 13.88 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:18:42.19 +68:06:24.5: 13.95 +/- 0.05 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:36:23.83 +68:50:09.1: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.03
Forced photometry filter KEPT candidate at 09:18:42.19 +68:06:24.5: ref_mag=13.95 +/- 0.03 new_mean_mag=12.9631 delta=0.98 (need > 0.90)
Forced photometry reference-image weighted average: 13.84 +/- 0.03
Forced photometry filter REJECTED candidate at 09:36:23.83 +68:50:09.1: ref_mag=13.84 +/- 0.03 new_mean_mag=12.9406 delta=0.90 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:48:33.28 +69:08:54.5: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.03
Forced photometry filter KEPT candidate at 09:48:33.28 +69:08:54.5: ref_mag=13.84 +/- 0.03 new_mean_mag=12.8675 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:01:00.51 +66:53:49.0: 13.87 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:34:30.35 +68:23:33.0: 13.88 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:01:00.51 +66:53:49.0: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Forced photometry filter KEPT candidate at 09:01:00.51 +66:53:49.0: ref_mag=13.86 +/- 0.03 new_mean_mag=12.8825 delta=0.98 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:34:30.35 +68:23:33.0: 13.83 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Forced photometry filter KEPT candidate at 09:34:30.35 +68:23:33.0: ref_mag=13.85 +/- 0.03 new_mean_mag=12.8880 delta=0.96 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:33:38.33 +68:29:53.8: 13.85 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:29:00.64 +69:19:07.4: 13.82 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:24:05.08 +68:11:42.6: 13.84 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:33:30.84 +70:35:10.7: 13.78 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-01_20.00sec_-15.00C_LIGHT_0292.fits at 09:16:28.46 +68:06:51.0: 13.78 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:33:38.33 +68:29:53.8: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Forced photometry filter KEPT candidate at 09:33:38.33 +68:29:53.8: ref_mag=13.83 +/- 0.03 new_mean_mag=12.9122 delta=0.92 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:29:00.64 +69:19:07.4: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 09:29:00.64 +69:19:07.4: ref_mag=13.79 +/- 0.03 new_mean_mag=12.8203 delta=0.97 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:24:05.08 +68:11:42.6: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Forced photometry filter KEPT candidate at 09:24:05.08 +68:11:42.6: ref_mag=13.91 +/- 0.03 new_mean_mag=12.9363 delta=0.97 (need > 0.90)
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:33:30.84 +70:35:10.7: 13.79 +/- 0.04 detection
Forced photometry on wcs_UMa-01-Q1b1x1_2026-02-11_01-08-51_20.00sec_-15.00C_LIGHT_0293.fits at 09:16:28.46 +68:06:51.0: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 09:33:30.84 +70:35:10.7: ref_mag=13.79 +/- 0.03 new_mean_mag=12.8424 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Forced photometry filter KEPT candidate at 09:16:28.46 +68:06:51.0: ref_mag=13.78 +/- 0.03 new_mean_mag=12.8760 delta=0.90 (need > 0.90)
Adding exclusion_list_local.txt__out01085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51488.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 52s
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: 19s
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Considering the candidate 65661_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 65661_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
**** FOUND 08:32:41.47 +69:20:08.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 65760_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 65760_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
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Considering the candidate 65812_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 65812_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
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Considering the candidate 65834_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 65834_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
**** FOUND 08:34:24.89 +66:54:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65887_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 65887_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
**** FOUND 09:34:07.88 +69:50:59.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 66001_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 66001_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
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Considering the candidate 66072_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 66072_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
**** FOUND 09:08:05.48 +66:23:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66154_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 66154_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
Rejecting candidate due to large distance (25.4") between the two second-epoch detections
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Considering the candidate 51488_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 51488_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 46308_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 46308_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 01085_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 01085_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 28314_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 28314_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 30940_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 30940_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 23018_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 23018_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 49868_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 49868_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 28877_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 28877_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 10691_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 10691_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 49411_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 49411_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 50364_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 50364_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 45133_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 45133_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 50405_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 50405_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 07683_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 07683_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 39381_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 39381_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 04084_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 04084_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 39202_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 39202_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 47516_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 47516_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 41316_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 41316_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 07628_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 07628_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
**** FOUND 10:55:39.96 +71:52:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24456_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 24456_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 29358_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 29358_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 26501_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 26501_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 05806_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 05806_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 50726_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 50726_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 50681_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 50681_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 48692_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 48692_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 49388_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 49388_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 48993_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 48993_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 40532_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 40532_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 32172_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 32172_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 28536_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 28536_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 40489_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 40489_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 25922_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 25922_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
**** FOUND 08:52:15.16 +70:26:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47236_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 47236_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 22437_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 22437_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 24157_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 24157_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 43721_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 43721_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 46056_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 46056_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 31076_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 31076_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 47191_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 47191_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
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Considering the candidate 48578_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 48578_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 38848_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 38848_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
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Considering the candidate 30481_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 30481_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 23914_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
The candidate 23914_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326 did not pass the final checks
**** FOUND 10:44:38.03 +68:46:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41850_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 41850_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 50705_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 50705_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 51118_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 51118_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 30955_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 30955_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 49149_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 49149_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 48505_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 48505_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
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Considering the candidate 24398_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
Preparing report for the candidate 24398_fd_UMa-01-Q1b1x1_2026-09-15_03-42-47_20.00sec_-0.00C_LIGHTs_0326
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 74s
Prepared the HTML report for the field UMa-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:35:48.89 +74:00:32.5
10:31:12.34 +73:30:02.2
10:26:26.62 +73:16:57.3
10:32:14.30 +72:44:05.3
10:37:48.79 +71:56:03.4
10:11:42.07 +70:18:29.2
10:08:36.54 +70:15:28.1
09:38:15.28 +70:34:48.6
09:33:30.84 +70:35:10.7
09:35:48.66 +70:33:06.6
09:59:21.55 +69:44:07.7
09:41:17.54 +69:40:53.4
09:51:38.39 +69:28:28.4
09:49:40.64 +69:26:21.9
09:35:17.38 +69:33:29.1
09:48:33.28 +69:08:54.5
09:43:31.50 +69:08:03.6
09:29:00.64 +69:19:07.4
09:50:25.92 +68:59:15.1
09:26:48.82 +69:05:43.5
09:28:21.94 +68:55:53.8
09:25:39.10 +68:42:41.2
09:25:01.27 +68:55:21.8
09:15:23.55 +68:58:29.6
09:38:27.78 +68:43:33.7
09:01:00.51 +66:53:49.0
09:23:40.79 +68:51:26.7
09:15:54.48 +67:26:26.0
09:34:53.61 +67:26:17.7
09:26:23.20 +67:35:20.9
09:16:38.85 +67:52:01.8
09:19:11.27 +67:53:36.9
09:16:28.46 +68:06:51.0
09:18:42.19 +68:06:24.5
09:19:46.04 +68:07:36.8
09:24:10.59 +68:10:17.5
09:24:05.08 +68:11:42.6
09:41:07.10 +68:01:25.0
09:20:28.13 +68:16:51.4
09:14:11.92 +68:23:26.7
09:21:29.83 +68:26:22.8
09:26:01.17 +68:27:28.6
09:31:25.96 +68:25:19.2
09:34:30.35 +68:23:33.0
09:35:10.58 +68:22:38.9
09:33:38.33 +68:29:53.8
09:18:33.47 +68:41:51.1
########### Completed UMa-01-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 ####
09:18:33.47 +68:41:51.1
09:26:23.20 +67:35:20.9
10:35:48.89 +74:00:32.5
09:41:17.54 +69:40:53.4
09:43:31.50 +69:08:03.6
10:08:36.54 +70:15:28.1
09:14:11.92 +68:23:26.7
09:49:40.64 +69:26:21.9
10:37:48.79 +71:56:03.4
09:20:28.13 +68:16:51.4
09:21:29.83 +68:26:22.8
09:15:54.48 +67:26:26.0
09:26:01.17 +68:27:28.6
10:32:14.30 +72:44:05.3
09:25:39.10 +68:42:41.2
10:31:12.34 +73:30:02.2
09:28:21.94 +68:55:53.8
09:19:11.27 +67:53:36.9
09:38:27.78 +68:43:33.7
09:35:48.66 +70:33:06.6
09:35:17.38 +69:33:29.1
09:59:21.55 +69:44:07.7
10:26:26.62 +73:16:57.3
09:35:10.58 +68:22:38.9
09:31:25.96 +68:25:19.2
09:19:46.04 +68:07:36.8
09:41:07.10 +68:01:25.0
09:24:10.59 +68:10:17.5
09:15:23.55 +68:58:29.6
09:26:48.82 +69:05:43.5
09:51:38.39 +69:28:28.4
09:25:01.27 +68:55:21.8
09:16:38.85 +67:52:01.8
10:11:42.07 +70:18:29.2
09:38:15.28 +70:34:48.6
09:23:40.79 +68:51:26.7
09:34:53.61 +67:26:17.7
09:50:25.92 +68:59:15.1
09:18:42.19 +68:06:24.5
09:48:33.28 +69:08:54.5
09:01:00.51 +66:53:49.0
09:34:30.35 +68:23:33.0
09:33:38.33 +68:29:53.8
09:29:00.64 +69:19:07.4
09:24:05.08 +68:11:42.6
09:16:28.46 +68:06:51.0
09:33:30.84 +70:35:10.7
###################################################################################
09:18:33.47 +68:41:51.1 -- not an asteroid (will add it to exclusion list)
09:26:23.20 +67:35:20.9 -- not an asteroid (will add it to exclusion list)
10:35:48.89 +74:00:32.5 -- not an asteroid (will add it to exclusion list)
09:41:17.54 +69:40:53.4 -- not an asteroid (will add it to exclusion list)
09:43:31.50 +69:08:03.6 -- not an asteroid (will add it to exclusion list)
10:08:36.54 +70:15:28.1 -- not an asteroid (will add it to exclusion list)
09:14:11.92 +68:23:26.7 -- not an asteroid (will add it to exclusion list)
09:49:40.64 +69:26:21.9 -- not an asteroid (will add it to exclusion list)
10:37:48.79 +71:56:03.4 -- not an asteroid (will add it to exclusion list)
09:20:28.13 +68:16:51.4 -- not an asteroid (will add it to exclusion list)
09:21:29.83 +68:26:22.8 -- not an asteroid (will add it to exclusion list)
09:15:54.48 +67:26:26.0 -- not an asteroid (will add it to exclusion list)
09:26:01.17 +68:27:28.6 -- not an asteroid (will add it to exclusion list)
10:32:14.30 +72:44:05.3 -- not an asteroid (will add it to exclusion list)
09:25:39.10 +68:42:41.2 -- not an asteroid (will add it to exclusion list)
10:31:12.34 +73:30:02.2 -- not an asteroid (will add it to exclusion list)
09:28:21.94 +68:55:53.8 -- not an asteroid (will add it to exclusion list)
09:19:11.27 +67:53:36.9 -- not an asteroid (will add it to exclusion list)
09:38:27.78 +68:43:33.7 -- not an asteroid (will add it to exclusion list)
09:35:48.66 +70:33:06.6 -- not an asteroid (will add it to exclusion list)
09:35:17.38 +69:33:29.1 -- not an asteroid (will add it to exclusion list)
09:59:21.55 +69:44:07.7 -- not an asteroid (will add it to exclusion list)
10:26:26.62 +73:16:57.3 -- not an asteroid (will add it to exclusion list)
09:35:10.58 +68:22:38.9 -- not an asteroid (will add it to exclusion list)
09:31:25.96 +68:25:19.2 -- not an asteroid (will add it to exclusion list)
09:19:46.04 +68:07:36.8 -- not an asteroid (will add it to exclusion list)
09:41:07.10 +68:01:25.0 -- not an asteroid (will add it to exclusion list)
09:24:10.59 +68:10:17.5 -- not an asteroid (will add it to exclusion list)
09:15:23.55 +68:58:29.6 -- not an asteroid (will add it to exclusion list)
09:26:48.82 +69:05:43.5 -- not an asteroid (will add it to exclusion list)
09:51:38.39 +69:28:28.4 -- not an asteroid (will add it to exclusion list)
09:25:01.27 +68:55:21.8 -- not an asteroid (will add it to exclusion list)
09:16:38.85 +67:52:01.8 -- not an asteroid (will add it to exclusion list)
10:11:42.07 +70:18:29.2 -- not an asteroid (will add it to exclusion list)
09:38:15.28 +70:34:48.6 -- not an asteroid (will add it to exclusion list)
09:23:40.79 +68:51:26.7 -- not an asteroid (will add it to exclusion list)
09:34:53.61 +67:26:17.7 -- not an asteroid (will add it to exclusion list)
09:50:25.92 +68:59:15.1 -- not an asteroid (will add it to exclusion list)
09:18:42.19 +68:06:24.5 -- not an asteroid (will add it to exclusion list)
09:48:33.28 +69:08:54.5 -- not an asteroid (will add it to exclusion list)
09:01:00.51 +66:53:49.0 -- not an asteroid (will add it to exclusion list)
09:34:30.35 +68:23:33.0 -- not an asteroid (will add it to exclusion list)
09:33:38.33 +68:29:53.8 -- not an asteroid (will add it to exclusion list)
09:29:00.64 +69:19:07.4 -- not an asteroid (will add it to exclusion list)
09:24:05.08 +68:11:42.6 -- not an asteroid (will add it to exclusion list)
09:16:28.46 +68:06:51.0 -- not an asteroid (will add it to exclusion list)
09:33:30.84 +70:35:10.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
09:01:00.51 +66:53:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:14:11.92 +68:23:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:15:23.55 +68:58:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:15:54.48 +67:26:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:16:28.46 +68:06:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:16:38.85 +67:52:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:18:33.47 +68:41:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:18:42.19 +68:06:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:19:11.27 +67:53:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:19:46.04 +68:07:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:20:28.13 +68:16:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:29.83 +68:26:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:23:40.79 +68:51:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:24:05.08 +68:11:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:24:10.59 +68:10:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:25:01.27 +68:55:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:25:39.10 +68:42:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:26:01.17 +68:27:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:26:23.20 +67:35:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:26:48.82 +69:05:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:28:21.94 +68:55:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:00.64 +69:19:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:25.96 +68:25:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:33:30.84 +70:35:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:33:38.33 +68:29:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:34:30.35 +68:23:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:34:53.61 +67:26:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:35:10.58 +68:22:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:35:17.38 +69:33:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:35:48.66 +70:33:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:38:15.28 +70:34:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:38:27.78 +68:43:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:41:07.10 +68:01:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:41:17.54 +69:40:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:43:31.50 +69:08:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:48:33.28 +69:08:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:49:40.64 +69:26:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:50:25.92 +68:59:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:51:38.39 +69:28:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:59:21.55 +69:44:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:36.54 +70:15:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:42.07 +70:18:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:26:26.62 +73:16:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:31:12.34 +73:30:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:32:14.30 +72:44:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:35:48.89 +74:00:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:37:48.79 +71:56:03.4 -- 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)
09:01:00.51 +66:53:49.0 -- not a known variable star
09:14:11.92 +68:23:26.7 -- not a known variable star
09:15:23.55 +68:58:29.6 -- not a known variable star
09:15:54.48 +67:26:26.0 -- not a known variable star
09:16:28.46 +68:06:51.0 -- not a known variable star
09:16:38.85 +67:52:01.8 -- not a known variable star
09:18:33.47 +68:41:51.1 -- not a known variable star
09:18:42.19 +68:06:24.5 -- not a known variable star
09:19:11.27 +67:53:36.9 -- not a known variable star
09:19:46.04 +68:07:36.8 -- not a known variable star
09:20:28.13 +68:16:51.4 -- not a known variable star
09:21:29.83 +68:26:22.8 -- not a known variable star
09:23:40.79 +68:51:26.7 -- a known variable star
09:24:05.08 +68:11:42.6 -- not a known variable star
09:24:10.59 +68:10:17.5 -- not a known variable star
09:25:01.27 +68:55:21.8 -- not a known variable star
09:25:39.10 +68:42:41.2 -- not a known variable star
09:26:01.17 +68:27:28.6 -- not a known variable star
09:26:23.20 +67:35:20.9 -- not a known variable star
09:26:48.82 +69:05:43.5 -- not a known variable star
09:28:21.94 +68:55:53.8 -- not a known variable star
09:29:00.64 +69:19:07.4 -- not a known variable star
09:31:25.96 +68:25:19.2 -- not a known variable star
09:33:30.84 +70:35:10.7 -- not a known variable star
09:33:38.33 +68:29:53.8 -- not a known variable star
09:34:30.35 +68:23:33.0 -- not a known variable star
09:34:53.61 +67:26:17.7 -- not a known variable star
09:35:10.58 +68:22:38.9 -- not a known variable star
09:35:17.38 +69:33:29.1 -- not a known variable star
09:35:48.66 +70:33:06.6 -- not a known variable star
09:38:15.28 +70:34:48.6 -- not a known variable star
09:38:27.78 +68:43:33.7 -- not a known variable star
09:41:07.10 +68:01:25.0 -- not a known variable star
09:41:17.54 +69:40:53.4 -- not a known variable star
09:43:31.50 +69:08:03.6 -- not a known variable star
09:48:33.28 +69:08:54.5 -- not a known variable star
09:49:40.64 +69:26:21.9 -- not a known variable star
09:50:25.92 +68:59:15.1 -- not a known variable star
09:51:38.39 +69:28:28.4 -- not a known variable star
09:59:21.55 +69:44:07.7 -- not a known variable star
10:08:36.54 +70:15:28.1 -- not a known variable star
10:11:42.07 +70:18:29.2 -- not a known variable star
10:26:26.62 +73:16:57.3 -- not a known variable star
10:31:12.34 +73:30:02.2 -- not a known variable star
10:32:14.30 +72:44:05.3 -- not a known variable star
10:35:48.89 +74:00:32.5 -- a known variable star
10:37:48.79 +71:56:03.4 -- not a known variable star
Found 45 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
47 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
09:01:00.51 +66:53:49.0
09:14:11.92 +68:23:26.7
09:15:23.55 +68:58:29.6
09:15:54.48 +67:26:26.0
09:16:28.46 +68:06:51.0
09:16:38.85 +67:52:01.8
09:18:33.47 +68:41:51.1
09:18:42.19 +68:06:24.5
09:19:11.27 +67:53:36.9
09:19:46.04 +68:07:36.8
09:20:28.13 +68:16:51.4
09:21:29.83 +68:26:22.8
09:23:40.79 +68:51:26.7
09:24:05.08 +68:11:42.6
09:24:10.59 +68:10:17.5
09:25:01.27 +68:55:21.8
09:25:39.10 +68:42:41.2
09:26:01.17 +68:27:28.6
09:26:23.20 +67:35:20.9
09:26:48.82 +69:05:43.5
09:28:21.94 +68:55:53.8
09:29:00.64 +69:19:07.4
09:31:25.96 +68:25:19.2
09:33:30.84 +70:35:10.7
09:33:38.33 +68:29:53.8
09:34:30.35 +68:23:33.0
09:34:53.61 +67:26:17.7
09:35:10.58 +68:22:38.9
09:35:17.38 +69:33:29.1
09:35:48.66 +70:33:06.6
09:38:15.28 +70:34:48.6
09:38:27.78 +68:43:33.7
09:41:07.10 +68:01:25.0
09:41:17.54 +69:40:53.4
09:43:31.50 +69:08:03.6
09:48:33.28 +69:08:54.5
09:49:40.64 +69:26:21.9
09:50:25.92 +68:59:15.1
09:51:38.39 +69:28:28.4
09:59:21.55 +69:44:07.7
10:08:36.54 +70:15:28.1
10:11:42.07 +70:18:29.2
10:26:26.62 +73:16:57.3
10:31:12.34 +73:30:02.2
10:32:14.30 +72:44:05.3
10:35:48.89 +74:00:32.5
10:37:48.79 +71:56:03.4
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461298.86253920 -observatory V36
12:27:16.74 -02:43:51.6 Mercury (-0.5mag)
13:54:21.53 -17:19:56.5 Venus (-4.8mag)
07:35:28.06 +22:23:24.6 Mars (1.2mag)
09:15:33.99 +16:29:38.8 Jupiter (-1.8mag)
00:49:45.42 +02:24:51.3 Saturn (0.4mag)
04:13:40.32 +21:01:57.7 Uranus (5.7mag)
00:12:57.83 -00:08:28.8 Neptune (7.7mag)
20:25:04.99 -23:41:15.6 Pluto (14.5mag)
14:35:41.09 -20:48:27.8 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 362 Sep 15 03:45 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461298.86253920:
09:15:34.96 +16:29:35.3 Io (6.0mag)
09:15:27.10 +16:30:14.4 Europa (6.2mag)
09:15:31.49 +16:29:51.0 Ganymede (5.6mag)
09:16:02.52 +16:27:15.8 Callisto (6.8mag)
09:13:39.61 +16:49:16.6 Himalia (15.7mag)
09:15:38.18 +16:29:19.1 Thebe (16.5mag)
09:13:10.18 +16:43:16.9 Elara (17.7mag)
09:19:14.18 +15:55:03.4 Pasiphae (17.9mag)
09:16:03.85 +16:49:39.5 Carme (18.9mag)
00:49:48.53 +02:24:14.5 Titan (8.3mag)
00:49:41.21 +02:24:56.2 Rhea (9.6mag)
00:49:37.46 +02:26:15.6 Iapetus (11.0mag)
00:49:40.23 +02:25:14.3 Hyperion (14.3mag)
00:48:24.14 +02:13:53.5 Phoebe (16.3mag)
-rw-r--r-- 1 apache apache 568 Sep 15 03:45 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461298.86253920:
23:11:28.71 +09:02:18.8 JWST
17:51:46.70 +30:26:04.3 Chandra
11:53:11.07 -61:13:58.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 15 03:45 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461298.86253920 -observatory V36
03:44:28.60 +19:40:30.7 17.3mag P/1996 R2 (Lagerkvist)
18:06:20.25 -34:03:26.5 14.4mag P/2010 H2 (Vales)
07:25:19.29 -70:45:43.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:16:25.44 +33:54:49.4 17.7mag C/2017 K2 (PANSTARRS)
22:07:15.44 +27:38:35.8 17.5mag C/2022 E2 (ATLAS)
07:16:01.84 +25:49:55.5 16.9mag C/2022 N2 (PANSTARRS)
10:56:53.63 +26:57:06.3 17.1mag C/2022 QE78 (ATLAS)
09:53:43.12 +05:11:14.9 18.0mag C/2022 R6 (PANSTARRS)
15:27:52.38 -16:21:15.8 15.0mag C/2023 R1 (PANSTARRS)
08:45:09.43 +33:25:10.2 15.9mag C/2024 E1 (Wierzchos)
15:07:51.21 +15:14:03.0 17.9mag C/2024 G6 (ATLAS)
18:29:20.23 +42:49:36.6 13.7mag C/2024 J3 (ATLAS)
20:15:38.18 +48:46:49.7 17.4mag C/2024 R4 (PANSTARRS)
05:39:32.29 -13:08:59.7 15.0mag C/2024 T5 (ATLAS)
07:13:59.99 +16:53:50.7 17.8mag C/2025 J1 (Borisov)
11:31:11.30 +18:07:50.8 16.7mag C/2025 V2 (Rankin)
13:26:27.28 -00:32:31.1 16.7mag C/2025 Y1 (ATLAS)
17:04:39.93 +72:35:28.5 15.9mag C/2026 A2 (Bok)
03:00:59.77 +45:48:04.7 17.5mag C/2026 B2 (Sun-Gao)
12:20:48.32 +11:56:33.7 17.6mag A/2026 E1
22:32:48.06 -35:12:54.2 13.6mag 10P/Tempel
01:32:03.64 +38:28:56.7 17.6mag 11P/Tempel-Swift-LINEAR
11:53:36.15 -06:04:59.0 16.3mag 29P/Schwassmann-Wachmann
12:24:48.58 -07:37:27.1 17.7mag 63P/Wild
06:54:29.25 +18:35:38.0 17.1mag 78P/Gehrels
03:16:39.67 +15:02:18.5 17.2mag 88P/Howell
06:05:31.86 +31:39:41.4 17.3mag 112P/Urata-Niijima
07:55:13.75 +22:37:52.4 17.9mag 114P/Wiseman-Skiff
10:45:44.99 +19:07:47.9 14.8mag 123P/West-Hartley
13:04:36.43 -24:06:09.6 17.5mag 124P/Mrkos
06:26:49.11 +20:22:13.7 15.8mag 128P/Shoemaker-Holt
01:52:00.29 -16:07:51.4 14.6mag 161P/Hartley-IRAS
09:31:42.33 +09:30:31.7 12.4mag 169P/NEAT
03:29:57.63 +07:43:59.0 14.6mag 220P/McNaught
05:09:12.48 +38:44:19.7 15.3mag 260P/McNaught
08:53:03.02 +34:47:30.0 17.3mag 295P/LINEAR
15:30:44.34 -01:08:53.3 17.9mag 391P/Kowalski
09:34:39.53 +16:26:27.7 17.8mag 450P/LONEOS
-rw-r--r-- 1 apache apache 1.9K Sep 15 03:45 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
04:59:14.53 -83:27:58.80 ASASSN-26fd 2026-09-9.11 17.27
17:52:06.79 -23:43:20.70 ASASSN-26fc 2026-09-8.79 12.14
03:52:53.26 -14:19:28.70 SN 2026zfw 2026-09-8 17.78
01:53:26.46 +10:07:25.10 SN2026aacj 2026-09-7.17 16.27
20:04:34.47 +62:38:38.10 SN2026zji 2026-09-7.14 15.87
22:37:05.64 +34:24:35.00 SN2026aaiv 2026-09-7.25 13.48
22:24:21.29 -10:25:31.60 ASASSN-26fb 2026-09-5.3 13.93
00:44:54.28 +41:33:10.50 AT2026aabo 2026-09-3.29 15.02
00:52:12.40 -58:22:08.60 SN 2026zhl 2026-08-31.92 16.51
19:53:57.87 +61:00:19.70 ASASSN-26fa 2026-08-31.18 14.63
00:21:50.96 -09:29:16.30 AT2026zwp 2026-08-31.41 15.59
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
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
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
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
-rw-r--r-- 1 apache apache 5.7K Sep 15 03:45 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
00:42:12.76 +41:16:28.4 PNV J00421276+4116284 2026-09-10.9176 18.67Cmag
17:52:06.80 -23:43:20.7 TCP J17520680-2343207 2026-09-08.7896 12.6mag
-rw-r--r-- 1 apache apache 190K Sep 15 03:45 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
01:42:26.979 +05:55:55.63 AT 2026zoy 2026-08-23.35 19.3897
14:41:50.156 -12:29:45.38 AT 2026zox 2026-08-23.39 19.54
18:13:38.090 +02:40:52.69 AT 2026zow 2026-08-23.42 19.03
02:06:52.332 -32:11:09.26 AT 2026zov 2026-08-07.72 20.15
03:27:15.082 -01:34:39.09 AT 2026zou 2026-08-07.78 20.12
07:25:07.240 -63:32:13.96 AT 2026zot 2026-08-23.12 18.353
16:56:50.544 +62:27:16.42 AT 2026zos 2026-08-14.94 18.874
19:11:34.945 -61:49:22.06 AT 2026zor 2026-08-22.85 18.462
03:29:28.370 -52:45:10.95 AT 2026zoq 2026-08-23.07 18.492
20:58:37.510 -60:29:13.04 AT 2026zop 2026-08-22.92 18.795
15:42:39.532 +45:40:22.19 AT 2026zoo 2026-08-20.91 18.832
05:33:32.309 -63:42:42.28 AT 2026zon 2026-08-23.09 18.975
23:30:20.920 -22:10:13.01 AT 2026zom 2026-08-16.39 19.5605
00:48:00.910 +25:04:50.63 AT 2026zol 2026-08-15.40 21.0878
00:01:16.883 +11:49:46.14 AT 2026zoj 2026-08-22.22 20.25
15:52:11.006 -06:28:01.00 AT 2026zoi 2026-08-23.37 18.48
03:31:11.092 -14:38:09.71 AT 2026zoh 2026-08-19.79 20.03
21:18:35.112 -33:20:37.95 AT 2026zog 2026-08-20.54 19.38
02:00:38.724 -25:30:59.99 AT 2026zof 2026-08-22.74 20.44
03:40:37.734 -13:59:47.56 AT 2026zoe 2026-08-22.77 20.28
-rw-r--r-- 1 apache apache 89K Sep 15 03:45 tns_transients_list.txt
