This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.43 13:34:41.89 +54:41:13.1
109.86559 61.33023 galactic UMa Second-epoch detections are separated by 0.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1561974847009535744 | 13:34:41.87 +54:41:13.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.238+/-0.026 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:34:41.89 +54:41:13.1: 11.46 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:34:41.89 +54:41:13.1: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 34 41.89 +54 41 13.1 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1561974847009535744,2461258.6988,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1561974847009535744 20260806.1988 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.57 13:25:55.53 +54:55:18.2
112.52821 61.50444 galactic UMa Second-epoch detections are separated by 0.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565077153427131520 | 13:25:55.52 +54:55:18.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.254+/-0.031 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:25:55.53 +54:55:18.2: 11.49 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:25:55.53 +54:55:18.2: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 25 55.53 +54 55 18.2 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565077153427131520,2461258.6988,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565077153427131520 20260806.1988 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.38 13:30:14.92 +56:36:07.6
112.32988 59.72011 galactic UMa Second-epoch detections are separated by 0.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565642680360344320 | 13:30:14.94 +56:36:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.376+/-0.034 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:30:14.92 +56:36:07.6: 11.49 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:30:14.92 +56:36:07.6: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 30 14.92 +56 36 07.6 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565642680360344320,2461258.6988,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565642680360344320 20260806.1988 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.37 13:31:15.03 +57:33:48.2
112.63409 58.76179 galactic UMa Second-epoch detections are separated by 0.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565806331499186176 | 13:31:15.05 +57:33:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.374+/-0.025 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:31:15.03 +57:33:48.2: 11.50 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:31:15.03 +57:33:48.2: 11.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 31 15.03 +57 33 48.2 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565806331499186176,2461258.6988,10.37,0.05,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 1565806331499186176 20260806.1988 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.42 13:26:02.28 +57:11:14.2
113.74099 59.31929 galactic UMa Second-epoch detections are separated by 0.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565876532739593600 | 13:26:02.41 +57:11:13.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:26:02.28 +57:11:14.2: 11.53 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:26:02.28 +57:11:14.2: 11.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 26 02.28 +57 11 14.2 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565876532739593600,2461258.6988,10.42,0.05,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 1565876532739593600 20260806.1988 10.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.55 13:15:30.00 +58:34:02.4
116.96524 58.28130 galactic UMa Second-epoch detections are separated by 0.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566984118905424128 | 13:15:29.99 +58:34:02.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.292+/-0.030 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:15:30.00 +58:34:02.4: 11.53 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:15:30.00 +58:34:02.4: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 15 30.00 +58 34 02.4 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566984118905424128,2461258.6988,10.55,0.05,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 1566984118905424128 20260806.1988 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.38 13:33:48.65 +56:21:08.6
111.24739 59.80425 galactic UMa Second-epoch detections are separated by 0.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565580111276704384 | 13:33:48.67 +56:21:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.655+/-0.030 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:33:48.65 +56:21:08.6: 11.57 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:33:48.65 +56:21:08.6: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 33 48.65 +56 21 08.6 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565580111276704384,2461258.6988,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565580111276704384 20260806.1988 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.51 13:19:45.22 +57:36:44.1
115.54487 59.10804 galactic UMa Second-epoch detections are separated by 0.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566332967504698112 | 13:19:45.23 +57:36:43.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.390+/-0.028 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:19:45.22 +57:36:44.1: 11.57 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:19:45.22 +57:36:44.1: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 19 45.22 +57 36 44.1 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566332967504698112,2461258.6988,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1566332967504698112 20260806.1988 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.49 13:27:59.91 +56:39:40.6
112.95154 59.75292 galactic UMa Second-epoch detections are separated by 0.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565845334097107840 | 13:27:59.96 +56:39:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.349+/-0.033 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:27:59.91 +56:39:40.6: 11.58 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:27:59.91 +56:39:40.6: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 27 59.91 +56 39 40.6 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565845334097107840,2461258.6988,10.49,0.05,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 1565845334097107840 20260806.1988 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.52 13:30:16.46 +55:57:24.3
111.93507 60.33461 galactic UMa Second-epoch detections are separated by 0.6" and 8.5 pix
The object was found in VSX 0" ASASSN-V J133016.45+555724.4
Type: EA
# Max. Min./Amp. JD0 Period
11.550 V 11.670 V 2457402.07800 2.421770000000
The object was not found in astcheck.
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:30:16.46 +55:57:24.3: 11.58 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:30:16.46 +55:57:24.3: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 30 16.46 +55 57 24.3 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J133016.45+555724.4,2461258.6988,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J133016.45+555724.4 20260806.1988 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.60 13:24:40.14 +55:43:16.2
113.33448 60.78356 galactic UMa Second-epoch detections are separated by 0.1" and 8.4 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 | ASASSN-V J132436.03+554248.6 | 13:24:36.00 +55:42:48.5 (Gaia DR3) | ROT (local) | 6.270500000000 (local) | Gaia3var=VARIABLE SpType: K1 (LAMOST DR5) J-Ks=0.382+/-0.033 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:24:40.14 +55:43:16.2: 11.61 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:24:40.14 +55:43:16.2: 11.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 24 40.14 +55 43 16.2 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J132436.03+554248.6,2461258.6988,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J132436.03+554248.6 20260806.1988 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.52 13:25:48.19 +57:15:25.8
113.83681 59.26013 galactic UMa Second-epoch detections are separated by 0.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565877941488870272 | 13:25:48.26 +57:15:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.410+/-0.032 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:25:48.19 +57:15:25.8: 11.63 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:25:48.19 +57:15:25.8: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 25 48.19 +57 15 25.8 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565877941488870272,2461258.6988,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565877941488870272 20260806.1988 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.56 13:34:20.56 +54:34:42.8
109.88769 61.44977 galactic UMa Second-epoch detections are separated by 0.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562019171072027904 | 13:34:20.58 +54:34:42.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.393+/-0.027 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:34:20.56 +54:34:42.8: 11.62 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:34:20.56 +54:34:42.8: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 34 20.56 +54 34 42.8 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562019171072027904,2461258.6988,10.56,0.05,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 1562019171072027904 20260806.1988 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.57 13:34:29.99 +54:15:13.6
109.60443 61.74616 galactic UMa Second-epoch detections are separated by 0.5" and 8.6 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 | ATO J203.6227+54.2518 | 13:34:30.19 +54:15:16.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:34:29.99 +54:15:13.6: 11.63 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:34:29.99 +54:15:13.6: 11.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 34 29.99 +54 15 13.6 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J203.6227+54.2518,2461258.6988,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J203.6227+54.2518 20260806.1988 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.69 13:23:16.05 +56:22:41.7
114.05963 60.19834 galactic UMa Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565495689399814656 | 13:23:16.04 +56:22:42.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.371+/-0.026 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:23:16.05 +56:22:41.7: 11.65 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:23:16.05 +56:22:41.7: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 23 16.05 +56 22 41.7 10.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565495689399814656,2461258.6988,10.69,0.05,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
Gaia DR3 1565495689399814656 20260806.1988 10.69CV 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 08 06.1988 2461258.6988 10.71 13:34:27.04 +53:08:32.6
108.76607 62.78687 galactic UMa Second-epoch detections are separated by 0.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1560180409673569152 | 13:34:27.03 +53:08:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.403+/-0.031 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:34:27.04 +53:08:32.6: 11.66 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:34:27.04 +53:08:32.6: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 34 27.04 +53 08 32.6 10.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1560180409673569152,2461258.6988,10.71,0.05,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 1560180409673569152 20260806.1988 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.64 13:29:45.28 +54:22:32.6
111.07146 61.86138 galactic UMa Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565001145392249728 | 13:29:45.32 +54:22:33.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.548+/-0.026 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:29:45.28 +54:22:32.6: 11.70 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:29:45.28 +54:22:32.6: 11.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 29 45.28 +54 22 32.6 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565001145392249728,2461258.6988,10.64,0.05,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 1565001145392249728 20260806.1988 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.55 13:28:11.42 +57:27:17.9
113.33577 58.98330 galactic UMa Second-epoch detections are separated by 0.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565895705473553920 | 13:28:11.47 +57:27:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.370+/-0.031 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:28:11.42 +57:27:17.9: 11.70 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:28:11.42 +57:27:17.9: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 28 11.42 +57 27 17.9 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565895705473553920,2461258.6988,10.55,0.05,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 1565895705473553920 20260806.1988 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.62 13:17:30.73 +57:37:26.8
116.12211 59.15807 galactic UMa Second-epoch detections are separated by 0.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566377016688856192 | 13:17:30.74 +57:37:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.789+/-0.024 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:17:30.73 +57:37:26.8: 11.72 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:17:30.73 +57:37:26.8: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 17 30.73 +57 37 26.8 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566377016688856192,2461258.6988,10.62,0.05,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
Gaia DR3 1566377016688856192 20260806.1988 10.62CV 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 08 06.1988 2461258.6988 9.27 13:31:31.66 +57:20:57.0
112.44166 58.95513 galactic UMa Second-epoch detections are separated by 0.4" and 8.4 pix
The object was found in VSX 1" Gaia DR3 1565794997080346752
Type: RS
# Max. Min./Amp. JD0 Period
10.040 G 10.120 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:31:31.66 +57:20:57.0: 10.20 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:31:31.66 +57:20:57.0: 10.19 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.19 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 31 31.66 +57 20 57.0 9.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565794997080346752,2461258.6988,9.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565794997080346752 20260806.1988 9.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 9.48 13:36:04.83 +55:33:13.9
110.10618 60.44884 galactic UMa Second-epoch detections are separated by 0.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562164066087311744 | 13:36:04.84 +55:33:14.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.629+/-0.028 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:36:04.83 +55:33:13.9: 10.47 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:36:04.83 +55:33:13.9: 10.46 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.47 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 36 04.83 +55 33 13.9 9.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562164066087311744,2461258.6988,9.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1562164066087311744 20260806.1988 9.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.69 13:30:19.90 +56:33:19.9
112.28068 59.76118 galactic UMa Second-epoch detections are separated by 0.2" and 8.4 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 | ATO J202.5828+56.5555 | 13:30:19.88 +56:33:20.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.324+/-0.034 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:30:19.90 +56:33:19.9: 11.95 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:30:19.90 +56:33:19.9: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 30 19.90 +56 33 19.9 10.7 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
ATO J202.5828+56.5555,2461258.6988,10.69,0.05,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
ATO J202.5828+56.5555 20260806.1988 10.69CV 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 08 06.1988 2461258.6988 9.60 13:31:13.88 +56:14:46.3
111.85737 60.01824 galactic UMa Second-epoch detections are separated by 0.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565587017584600832 | 13:31:13.89 +56:14:46.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.607+/-0.028 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:31:13.88 +56:14:46.3: 10.59 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:31:13.88 +56:14:46.3: 10.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.59 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 31 13.88 +56 14 46.3 9.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565587017584600832,2461258.6988,9.60,0.05,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 1565587017584600832 20260806.1988 9.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 9.72 13:25:43.05 +57:29:37.5
113.97801 59.03461 galactic UMa Second-epoch detections are separated by 0.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565951746207341568 | 13:25:43.07 +57:29:37.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.631+/-0.030 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:25:43.05 +57:29:37.5: 10.68 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:25:43.05 +57:29:37.5: 10.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.70 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 25 43.05 +57 29 37.5 9.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565951746207341568,2461258.6988,9.72,0.05,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
Gaia DR3 1565951746207341568 20260806.1988 9.72CV 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 08 06.1988 2461258.6988 9.70 13:36:16.05 +56:34:35.0
110.76193 59.48006 galactic UMa Second-epoch detections are separated by 0.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562607925188864896 | 13:36:16.07 +56:34:35.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.435+/-0.028 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:36:16.05 +56:34:35.0: 10.73 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:36:16.05 +56:34:35.0: 10.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.73 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 36 16.05 +56 34 35.0 9.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562607925188864896,2461258.6988,9.70,0.05,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 1562607925188864896 20260806.1988 9.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 9.72 13:29:48.87 +57:29:40.5
112.95140 58.88385 galactic UMa Second-epoch detections are separated by 0.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565986930578679680 | 13:29:48.91 +57:29:40.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.630+/-0.029 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:29:48.87 +57:29:40.5: 10.75 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:29:48.87 +57:29:40.5: 10.74 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.75 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 29 48.87 +57 29 40.5 9.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565986930578679680,2461258.6988,9.72,0.05,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
Gaia DR3 1565986930578679680 20260806.1988 9.72CV 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 08 06.1988 2461258.6988 9.87 13:33:46.98 +55:05:27.0
110.40882 60.99591 galactic UMa Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562136234700609664 | 13:33:46.96 +55:05:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.322+/-0.031 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:33:46.98 +55:05:27.0: 10.80 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:33:46.98 +55:05:27.0: 10.80 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.80 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 33 46.98 +55 05 27.0 9.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562136234700609664,2461258.6988,9.87,0.05,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 1562136234700609664 20260806.1988 9.87CV 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 08 06.1988 2461258.6988 9.92 13:22:49.06 +57:08:53.9
114.55173 59.46647 galactic UMa Second-epoch detections are separated by 0.1" and 8.3 pix
The object was found in VSX 1" Gaia DR3 1565556093819891456
Type: ROT
# Max. Min./Amp. JD0 Period
10.690 G 10.730 G G
The object was not found in astcheck.
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:22:49.06 +57:08:53.9: 10.84 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:22:49.06 +57:08:53.9: 10.83 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.84 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 22 49.06 +57 08 53.9 9.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565556093819891456,2461258.6988,9.92,0.05,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 1565556093819891456 20260806.1988 9.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 9.86 13:35:47.98 +56:25:26.9
110.77969 59.64518 galactic UMa Second-epoch detections are separated by 0.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562605073330242176 | 13:35:47.93 +56:25:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.257+/-0.029 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:35:47.98 +56:25:26.9: 10.88 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:35:47.98 +56:25:26.9: 10.86 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 35 47.98 +56 25 26.9 9.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562605073330242176,2461258.6988,9.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1562605073330242176 20260806.1988 9.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 9.85 13:29:39.32 +57:46:53.7
113.14861 58.61486 galactic UMa Second-epoch detections are separated by 0.5" and 8.4 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 | ATO J202.4263+57.7850 | 13:29:39.26 +57:46:53.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.286+/-0.030 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:29:39.32 +57:46:53.7: 10.89 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:29:39.32 +57:46:53.7: 10.89 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.89 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 29 39.32 +57 46 53.7 9.8 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
ATO J202.4263+57.7850,2461258.6988,9.85,0.05,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
ATO J202.4263+57.7850 20260806.1988 9.85CV 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
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 9.88 13:37:33.57 +57:53:54.2
111.31004 58.17707 galactic UMa Second-epoch detections are separated by 0.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1661856888457841152 | 13:37:33.61 +57:53:53.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.392+/-0.027 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:37:33.57 +57:53:54.2: 10.95 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:37:33.57 +57:53:54.2: 10.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.95 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 37 33.57 +57 53 54.2 9.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1661856888457841152,2461258.6988,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1661856888457841152 20260806.1988 9.88CV 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 08 06.1988 2461258.6988 10.03 13:19:43.59 +57:38:24.6
115.56339 59.08155 galactic UMa Second-epoch detections are separated by 0.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566333104943652480 | 13:19:43.62 +57:38:24.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.799+/-0.035 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:19:43.59 +57:38:24.6: 10.98 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:19:43.59 +57:38:24.6: 10.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.98 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 19 43.59 +57 38 24.6 10.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566333104943652480,2461258.6988,10.03,0.05,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
Gaia DR3 1566333104943652480 20260806.1988 10.03CV 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 08 06.1988 2461258.6988 9.96 13:27:52.42 +56:39:14.1
112.98014 59.76479 galactic UMa Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565845368456846080 | 13:27:52.47 +56:39:14.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.869+/-0.037 (M)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:27:52.42 +56:39:14.1: 10.98 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:27:52.42 +56:39:14.1: 10.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.99 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 27 52.42 +56 39 14.1 10.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565845368456846080,2461258.6988,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565845368456846080 20260806.1988 9.96CV 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 08 06.1988 2461258.6988 9.95 13:30:35.53 +56:25:59.8
112.13955 59.86701 galactic UMa Second-epoch detections are separated by 0.1" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565636289448967424 | 13:30:35.56 +56:26:00.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.409+/-0.033 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:30:35.53 +56:25:59.8: 10.99 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:30:35.53 +56:25:59.8: 10.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.98 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 30 35.53 +56 25 59.8 9.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565636289448967424,2461258.6988,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565636289448967424 20260806.1988 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.06 13:29:49.51 +55:55:24.1
112.03593 60.38542 galactic UMa Second-epoch detections are separated by 0.4" and 8.4 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 | ATO J202.4692+55.9225 | 13:29:49.57 +55:55:24.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.404+/-0.026 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:29:49.51 +55:55:24.1: 11.06 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:29:49.51 +55:55:24.1: 11.03 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.05 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 29 49.51 +55 55 24.1 10.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J202.4692+55.9225,2461258.6988,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J202.4692+55.9225 20260806.1988 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.03 13:27:33.19 +57:11:01.1
113.35177 59.26782 galactic UMa Second-epoch detections are separated by 0.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565862788844217472 | 13:27:33.12 +57:11:01.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.312+/-0.031 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:27:33.19 +57:11:01.1: 11.06 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:27:33.19 +57:11:01.1: 11.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.06 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 27 33.19 +57 11 01.1 10.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565862788844217472,2461258.6988,10.03,0.05,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
Gaia DR3 1565862788844217472 20260806.1988 10.03CV 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 08 06.1988 2461258.6988 10.05 13:24:55.69 +58:02:03.5
114.43845 58.53827 galactic UMa Second-epoch detections are separated by 0.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566075132027142656 | 13:24:55.66 +58:02:04.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.360+/-0.026 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:24:55.69 +58:02:03.5: 11.07 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:24:55.69 +58:02:03.5: 11.10 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.08 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 24 55.69 +58 02 03.5 10.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566075132027142656,2461258.6988,10.05,0.05,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
Gaia DR3 1566075132027142656 20260806.1988 10.05CV 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 08 06.1988 2461258.6988 10.13 13:25:06.01 +56:03:55.8
113.40071 60.43547 galactic UMa Second-epoch detections are separated by 0.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565428378672738432 | 13:25:06.08 +56:03:55.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.347+/-0.028 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:25:06.01 +56:03:55.8: 11.09 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:25:06.01 +56:03:55.8: 11.10 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.10 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 25 06.01 +56 03 55.8 10.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565428378672738432,2461258.6988,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565428378672738432 20260806.1988 10.13CV 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 08 06.1988 2461258.6988 10.04 13:30:45.23 +56:10:21.4
111.93886 60.10862 galactic UMa Second-epoch detections are separated by 0.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565258160528753920 | 13:30:45.17 +56:10:22.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:30:45.23 +56:10:21.4: 11.12 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:30:45.23 +56:10:21.4: 11.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.10 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 30 45.23 +56 10 21.4 10.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565258160528753920,2461258.6988,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565258160528753920 20260806.1988 10.04CV 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 08 06.1988 2461258.6988 10.02 13:32:33.97 +58:04:59.5
112.61177 58.21340 galactic UMa Second-epoch detections are separated by 0.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565844062786729600 | 13:32:33.96 +58:04:59.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1956PMcCO..13a....B AG+58 893 J-Ks=0.290+/-0.030 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:32:33.97 +58:04:59.5: 11.12 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:32:33.97 +58:04:59.5: 11.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 32 33.97 +58 04 59.5 10.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565844062786729600,2461258.6988,10.02,0.05,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
Gaia DR3 1565844062786729600 20260806.1988 10.02CV 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 08 06.1988 2461258.6988 10.21 13:24:10.58 +55:55:38.0
113.58072 60.60268 galactic UMa Second-epoch detections are separated by 0.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565344094234235904 | 13:24:10.58 +55:55:37.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.344+/-0.032 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:24:10.58 +55:55:38.0: 11.17 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:24:10.58 +55:55:38.0: 11.18 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 24 10.58 +55 55 38.0 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565344094234235904,2461258.6988,10.21,0.05,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 1565344094234235904 20260806.1988 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.14 13:19:12.46 +57:54:48.1
115.80603 58.82904 galactic UMa Second-epoch detections are separated by 0.5" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566715666269729408 | 13:19:12.48 +57:54:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.334+/-0.028 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:19:12.46 +57:54:48.1: 11.18 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:19:12.46 +57:54:48.1: 11.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 19 12.46 +57 54 48.1 10.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566715666269729408,2461258.6988,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1566715666269729408 20260806.1988 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.17 13:34:38.50 +55:02:23.1
110.13455 61.00206 galactic UMa Second-epoch detections are separated by 0.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562126132936009984 | 13:34:38.61 +55:02:23.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:34:38.50 +55:02:23.1: 11.18 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:34:38.50 +55:02:23.1: 11.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 34 38.50 +55 02 23.1 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562126132936009984,2461258.6988,10.17,0.05,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 1562126132936009984 20260806.1988 10.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.24 13:35:00.05 +54:19:57.5
109.51881 61.64659 galactic UMa Second-epoch detections are separated by 0.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1561960931315525632 | 13:35:00.03 +54:19:57.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.376+/-0.030 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:35:00.05 +54:19:57.5: 11.19 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:35:00.05 +54:19:57.5: 11.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 35 00.05 +54 19 57.5 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1561960931315525632,2461258.6988,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1561960931315525632 20260806.1988 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.11 13:33:49.07 +57:11:48.0
111.77896 59.00449 galactic UMa Second-epoch detections are separated by 0.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565736551165343232 | 13:33:49.05 +57:11:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.413+/-0.033 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:33:49.07 +57:11:48.0: 11.22 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:33:49.07 +57:11:48.0: 11.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 33 49.07 +57 11 48.0 10.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565736551165343232,2461258.6988,10.11,0.05,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 1565736551165343232 20260806.1988 10.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.23 13:30:06.85 +55:32:44.9
111.72431 60.73290 galactic UMa Second-epoch detections are separated by 0.1" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565166351307843584 | 13:30:06.89 +55:32:45.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=0.912+/-0.052 (M)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:30:06.85 +55:32:44.9: 11.21 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:30:06.85 +55:32:44.9: 11.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 30 06.85 +55 32 44.9 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565166351307843584,2461258.6988,10.23,0.05,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 1565166351307843584 20260806.1988 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.18 13:33:07.59 +56:55:09.2
111.78155 59.29742 galactic UMa Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565633300151718784 | 13:33:07.62 +56:55:09.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.326+/-0.031 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:33:07.59 +56:55:09.2: 11.26 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:33:07.59 +56:55:09.2: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.26 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 33 07.59 +56 55 09.2 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565633300151718784,2461258.6988,10.18,0.05,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 1565633300151718784 20260806.1988 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.28 13:34:02.26 +53:45:49.8
109.37245 62.22864 galactic UMa Second-epoch detections are separated by 0.3" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1560420996561363712 | 13:34:02.26 +53:45:49.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.314+/-0.031 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:34:02.26 +53:45:49.8: 11.26 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:34:02.26 +53:45:49.8: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 34 02.26 +53 45 49.8 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1560420996561363712,2461258.6988,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1560420996561363712 20260806.1988 10.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.22 13:26:11.95 +58:08:48.1
114.18197 58.38713 galactic UMa Second-epoch detections are separated by 0.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566070837059822336 | 13:26:12.01 +58:08:48.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.294+/-0.030 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:26:11.95 +58:08:48.1: 11.32 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:26:11.95 +58:08:48.1: 11.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.32 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 26 11.95 +58 08 48.1 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566070837059822336,2461258.6988,10.22,0.05,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 1566070837059822336 20260806.1988 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.20 13:34:12.82 +57:23:34.5
111.80176 58.80143 galactic UMa Second-epoch detections are separated by 0.1" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565763111243112576 | 13:34:12.80 +57:23:35.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G9 (LAMOST DR5) J-Ks=0.519+/-0.027 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:34:12.82 +57:23:34.5: 11.36 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:34:12.82 +57:23:34.5: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 34 12.82 +57 23 34.5 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565763111243112576,2461258.6988,10.20,0.05,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 1565763111243112576 20260806.1988 10.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.36 13:21:34.24 +57:24:00.9
114.98884 59.26088 galactic UMa Second-epoch detections are separated by 0.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566314447605211904 | 13:21:34.23 +57:24:00.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.657+/-0.026 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:21:34.24 +57:24:00.9: 11.38 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:21:34.24 +57:24:00.9: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.39 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 21 34.24 +57 24 00.9 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566314447605211904,2461258.6988,10.36,0.05,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 1566314447605211904 20260806.1988 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.26 13:33:16.68 +56:02:20.7
111.18410 60.12464 galactic UMa Second-epoch detections are separated by 0.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565568806922771968 | 13:33:16.70 +56:02:20.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.624+/-0.029 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:33:16.68 +56:02:20.7: 11.38 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:33:16.68 +56:02:20.7: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.39 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 33 16.68 +56 02 20.7 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565568806922771968,2461258.6988,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565568806922771968 20260806.1988 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.40 13:22:34.87 +57:07:00.1
114.59826 59.50482 galactic UMa Second-epoch detections are separated by 0.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565556299977172608 | 13:22:34.90 +57:07:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.702+/-0.028 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:22:34.87 +57:07:00.1: 11.40 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:22:34.87 +57:07:00.1: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 22 34.87 +57 07 00.1 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565556299977172608,2461258.6988,10.40,0.05,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 1565556299977172608 20260806.1988 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.35 13:16:58.90 +57:58:46.2
116.39061 58.82316 galactic UMa Second-epoch detections are separated by 0.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566777685597522432 | 13:16:58.90 +57:58:46.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.552+/-0.026 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:16:58.90 +57:58:46.2: 11.42 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:16:58.90 +57:58:46.2: 11.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.40 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 16 58.90 +57 58 46.2 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566777685597522432,2461258.6988,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1566777685597522432 20260806.1988 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.30 13:32:12.73 +56:43:21.7
111.89417 59.52322 galactic UMa Second-epoch detections are separated by 0.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565670099431503616 | 13:32:12.76 +56:43:22.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.501+/-0.026 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:32:12.73 +56:43:21.7: 11.42 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:32:12.73 +56:43:21.7: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 32 12.73 +56 43 21.7 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565670099431503616,2461258.6988,10.30,0.05,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 1565670099431503616 20260806.1988 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.46 13:26:27.45 +55:31:27.0
112.72607 60.90476 galactic UMa Second-epoch detections are separated by 0.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565127937120460800 | 13:26:27.43 +55:31:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.293+/-0.035 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:26:27.45 +55:31:27.0: 11.42 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:26:27.45 +55:31:27.0: 11.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 26 27.45 +55 31 27.0 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565127937120460800,2461258.6988,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565127937120460800 20260806.1988 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.28 13:37:20.82 +57:42:57.3
111.24361 58.35839 galactic UMa Second-epoch detections are separated by 0.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1661836581852104192 | 13:37:20.72 +57:42:57.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.329+/-0.030 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:37:20.82 +57:42:57.3: 11.45 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:37:20.82 +57:42:57.3: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 37 20.82 +57 42 57.3 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1661836581852104192,2461258.6988,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1661836581852104192 20260806.1988 10.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.52 13:20:40.79 +56:16:55.4
114.71607 60.37730 galactic UMa Second-epoch detections are separated by 1.7" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565408724902177792 | 13:20:40.68 +56:16:55.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.585+/-0.028 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:20:40.79 +56:16:55.4: 11.46 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:20:40.79 +56:16:55.4: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 20 40.79 +56 16 55.4 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565408724902177792,2461258.6988,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565408724902177792 20260806.1988 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.32 13:32:35.65 +56:43:00.5
111.79240 59.51247 galactic UMa Second-epoch detections are separated by 0.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565624332259997312 | 13:32:35.61 +56:43:00.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.305+/-0.031 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:32:35.65 +56:43:00.5: 11.43 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:32:35.65 +56:43:00.5: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 32 35.65 +56 43 00.5 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565624332259997312,2461258.6988,10.32,0.05,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 1565624332259997312 20260806.1988 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.25 13:32:39.41 +56:21:47.7
111.55547 59.84529 galactic UMa Second-epoch detections are separated by 0.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565591862307226752 | 13:32:39.44 +56:21:48.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.790+/-0.033 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:32:39.41 +56:21:47.7: 11.40 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:32:39.41 +56:21:47.7: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.40 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 32 39.41 +56 21 47.7 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565591862307226752,2461258.6988,10.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565591862307226752 20260806.1988 10.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.32 13:29:32.26 +56:38:56.3
112.54253 59.70415 galactic UMa Second-epoch detections are separated by 0.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565654912427205888 | 13:29:32.25 +56:38:56.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.336+/-0.026 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:29:32.26 +56:38:56.3: 11.40 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:29:32.26 +56:38:56.3: 11.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.40 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 29 32.26 +56 38 56.3 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565654912427205888,2461258.6988,10.32,0.05,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 1565654912427205888 20260806.1988 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.30 13:27:36.74 +56:54:51.3
113.19129 59.52465 galactic UMa Second-epoch detections are separated by 0.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565852584001910400 | 13:27:36.78 +56:54:51.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.520+/-0.033 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:27:36.74 +56:54:51.3: 11.39 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:27:36.74 +56:54:51.3: 11.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 27 36.74 +56 54 51.3 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565852584001910400,2461258.6988,10.30,0.05,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 1565852584001910400 20260806.1988 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.40 13:16:26.33 +58:23:20.5
116.67360 58.43441 galactic UMa Second-epoch detections are separated by 0.2" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566791944888960384 | 13:16:26.31 +58:23:20.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.598+/-0.027 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:16:26.33 +58:23:20.5: 11.38 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:16:26.33 +58:23:20.5: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.39 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 16 26.33 +58 23 20.5 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566791944888960384,2461258.6988,10.40,0.05,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 1566791944888960384 20260806.1988 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.40 13:24:35.97 +55:42:48.2
113.34963 60.79364 galactic UMa Second-epoch detections are separated by 0.1" and 8.4 pix
The object was found in VSX 1" ASASSN-V J132436.03+554248.6
Type: ROT
# Max. Min./Amp. JD0 Period
11.280 V 11.380 V 2457002.12800 6.270500000000
The object was not found in astcheck.
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:24:35.97 +55:42:48.2: 11.34 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:24:35.97 +55:42:48.2: 11.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 24 35.97 +55 42 48.2 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J132436.03+554248.6,2461258.6988,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J132436.03+554248.6 20260806.1988 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.31 13:29:31.07 +54:28:48.1
111.20977 61.77308 galactic UMa Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565002798953203200 | 13:29:31.07 +54:28:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.366+/-0.028 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:29:31.07 +54:28:48.1: 11.29 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:29:31.07 +54:28:48.1: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 29 31.07 +54 28 48.1 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565002798953203200,2461258.6988,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565002798953203200 20260806.1988 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.17 13:35:42.07 +55:39:46.8
110.28466 60.36511 galactic UMa Second-epoch detections are separated by 0.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562543500678951936 | 13:35:42.12 +55:39:47.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.734+/-0.028 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:35:42.07 +55:39:46.8: 11.26 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:35:42.07 +55:39:46.8: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.26 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 35 42.07 +55 39 46.8 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562543500678951936,2461258.6988,10.17,0.05,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 1562543500678951936 20260806.1988 10.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.15 13:31:38.23 +57:46:45.5
112.66251 58.54027 galactic UMa Second-epoch detections are separated by 0.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565832998950310912 | 13:31:38.31 +57:46:46.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.428+/-0.028 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:31:38.23 +57:46:45.5: 11.26 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:31:38.23 +57:46:45.5: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 31 38.23 +57 46 45.5 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565832998950310912,2461258.6988,10.15,0.05,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 1565832998950310912 20260806.1988 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.17 13:35:17.16 +57:09:30.3
111.38950 58.97642 galactic UMa Second-epoch detections are separated by 0.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565733355709646592 | 13:35:17.19 +57:09:30.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.440+/-0.029 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:35:17.16 +57:09:30.3: 11.25 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:35:17.16 +57:09:30.3: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.26 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 35 17.16 +57 09 30.3 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565733355709646592,2461258.6988,10.17,0.05,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 1565733355709646592 20260806.1988 10.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.19 13:25:32.35 +57:02:27.0
113.79429 59.47834 galactic UMa Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565868320762573440 | 13:25:32.52 +57:02:27.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:25:32.35 +57:02:27.0: 11.22 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:25:32.35 +57:02:27.0: 11.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 25 32.35 +57 02 27.0 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565868320762573440,2461258.6988,10.19,0.05,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 1565868320762573440 20260806.1988 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.26 13:28:57.34 +54:55:28.8
111.65888 61.37483 galactic UMa Second-epoch detections are separated by 0.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565030733420988800 | 13:28:57.34 +54:55:29.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.241+/-0.032 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:28:57.34 +54:55:28.8: 11.18 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:28:57.34 +54:55:28.8: 11.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.18 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 28 57.34 +54 55 28.8 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565030733420988800,2461258.6988,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565030733420988800 20260806.1988 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.18 13:20:38.43 +58:20:20.3
115.62419 58.37303 galactic UMa Second-epoch detections are separated by 0.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566756519997968640 | 13:20:38.48 +58:20:20.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5) J-Ks=0.332+/-0.028 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:20:38.43 +58:20:20.3: 11.17 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:20:38.43 +58:20:20.3: 11.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.18 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 20 38.43 +58 20 20.3 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566756519997968640,2461258.6988,10.18,0.05,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 1566756519997968640 20260806.1988 10.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.19 13:17:31.54 +57:40:15.0
116.13660 59.11190 galactic UMa Second-epoch detections are separated by 0.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566383235801503616 | 13:17:31.50 +57:40:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1956PMcCO..13a....B AG+57 907 J-Ks=0.296+/-0.028 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:17:31.54 +57:40:15.0: 11.18 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:17:31.54 +57:40:15.0: 11.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 17 31.54 +57 40 15.0 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566383235801503616,2461258.6988,10.19,0.05,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 1566383235801503616 20260806.1988 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.16 13:32:12.43 +55:41:13.6
111.24234 60.50625 galactic UMa Second-epoch detections are separated by 0.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565181950629019264 | 13:32:12.48 +55:41:13.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5) J-Ks=0.450+/-0.026 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:32:12.43 +55:41:13.6: 11.17 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:32:12.43 +55:41:13.6: 11.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 32 12.43 +55 41 13.6 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565181950629019264,2461258.6988,10.16,0.05,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 1565181950629019264 20260806.1988 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.23 13:15:06.49 +58:19:32.4
116.98010 58.52822 galactic UMa Second-epoch detections are separated by 0.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566974532538792576 | 13:15:06.46 +58:19:32.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.239+/-0.025 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:15:06.49 +58:19:32.4: 11.16 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:15:06.49 +58:19:32.4: 11.15 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 15 06.49 +58 19 32.4 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566974532538792576,2461258.6988,10.23,0.05,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 1566974532538792576 20260806.1988 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.22 13:30:04.64 +54:05:47.9
110.78809 62.11118 galactic UMa Second-epoch detections are separated by 0.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1560493186372075648 | 13:30:04.71 +54:05:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.354+/-0.033 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:30:04.64 +54:05:47.9: 11.15 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:30:04.64 +54:05:47.9: 11.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.14 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 30 04.64 +54 05 47.9 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1560493186372075648,2461258.6988,10.22,0.05,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 1560493186372075648 20260806.1988 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.06 13:35:36.63 +56:26:44.6
110.84281 59.63371 galactic UMa Second-epoch detections are separated by 0.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562605348208149376 | 13:35:36.60 +56:26:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.227+/-0.028 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:35:36.63 +56:26:44.6: 11.13 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:35:36.63 +56:26:44.6: 11.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 35 36.63 +56 26 44.6 10.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562605348208149376,2461258.6988,10.06,0.05,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 1562605348208149376 20260806.1988 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.19 13:31:59.09 +53:43:16.7
109.95364 62.37339 galactic UMa Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J203.0009+53.7092 | 13:31:59.11 +53:43:16.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.590+/-0.031 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:31:59.09 +53:43:16.7: 11.12 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:31:59.09 +53:43:16.7: 11.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 31 59.09 +53 43 16.7 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J203.0009+53.7092,2461258.6988,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J203.0009+53.7092 20260806.1988 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.13 13:26:52.16 +56:17:06.8
113.04185 60.15749 galactic UMa Second-epoch detections are separated by 0.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565458340364158592 | 13:26:52.15 +56:17:06.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.292+/-0.026 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:26:52.16 +56:17:06.8: 11.12 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:26:52.16 +56:17:06.8: 11.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 26 52.16 +56 17 06.8 10.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565458340364158592,2461258.6988,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565458340364158592 20260806.1988 10.13CV 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 08 06.1988 2461258.6988 10.14 13:31:49.34 +54:25:39.5
110.50410 61.71544 galactic UMa Second-epoch detections are separated by 0.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562002231720966656 | 13:31:49.36 +54:25:39.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.683+/-0.027 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:31:49.34 +54:25:39.5: 11.10 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:31:49.34 +54:25:39.5: 11.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 31 49.34 +54 25 39.5 10.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562002231720966656,2461258.6988,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1562002231720966656 20260806.1988 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.06 13:26:07.48 +57:07:15.2
113.68452 59.38026 galactic UMa Second-epoch detections are separated by 0.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565870206251699456 | 13:26:07.48 +57:07:15.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.441+/-0.032 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:26:07.48 +57:07:15.2: 11.09 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:26:07.48 +57:07:15.2: 11.08 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.09 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 26 07.48 +57 07 15.2 10.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565870206251699456,2461258.6988,10.06,0.05,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 1565870206251699456 20260806.1988 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.16 13:29:41.46 +54:26:58.1
111.13905 61.79425 galactic UMa Second-epoch detections are separated by 0.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J202.4256+54.4602 | 13:29:41.47 +54:26:58.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.316+/-0.030 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:29:41.46 +54:26:58.1: 11.08 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:29:41.46 +54:26:58.1: 11.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.08 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 29 41.46 +54 26 58.1 10.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J202.4256+54.4602,2461258.6988,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J202.4256+54.4602 20260806.1988 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 9.96 13:35:29.99 +55:58:19.5
110.55177 60.08450 galactic UMa Second-epoch detections are separated by 0.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562565697070005376 | 13:35:29.99 +55:58:19.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.342+/-0.029 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:35:29.99 +55:58:19.5: 11.01 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:35:29.99 +55:58:19.5: 11.01 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.01 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 35 29.99 +55 58 19.5 10.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562565697070005376,2461258.6988,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1562565697070005376 20260806.1988 9.96CV 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 08 06.1988 2461258.6988 9.87 13:35:36.17 +57:42:23.5
111.65706 58.44450 galactic UMa Second-epoch detections are separated by 0.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565773758466098048 | 13:35:36.21 +57:42:23.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: Carbon (LAMOST DR5) J-Ks=0.674+/-0.029 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:35:36.17 +57:42:23.5: 10.99 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:35:36.17 +57:42:23.5: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.97 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 35 36.17 +57 42 23.5 9.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565773758466098048,2461258.6988,9.87,0.05,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 1565773758466098048 20260806.1988 9.87CV 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 08 06.1988 2461258.6988 10.03 13:23:06.20 +56:58:04.7
114.39168 59.63214 galactic UMa Second-epoch detections are separated by 0.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565537092884948992 | 13:23:06.25 +56:58:04.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.249+/-0.028 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:23:06.20 +56:58:04.7: 10.97 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:23:06.20 +56:58:04.7: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.97 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 23 06.20 +56 58 04.7 10.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565537092884948992,2461258.6988,10.03,0.05,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
Gaia DR3 1565537092884948992 20260806.1988 10.03CV 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 08 06.1988 2461258.6988 9.97 13:33:05.99 +56:01:54.6
111.22666 60.13956 galactic UMa Second-epoch detections are separated by 0.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565568669483818368 | 13:33:06.02 +56:01:54.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.337+/-0.030 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:33:05.99 +56:01:54.6: 10.97 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:33:05.99 +56:01:54.6: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.96 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 33 05.99 +56 01 54.6 10.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565568669483818368,2461258.6988,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565568669483818368 20260806.1988 9.97CV 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 08 06.1988 2461258.6988 10.01 13:30:08.92 +55:07:45.3
111.45082 61.12772 galactic UMa Second-epoch detections are separated by 0.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565050833867486464 | 13:30:08.93 +55:07:45.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.320+/-0.033 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:30:08.92 +55:07:45.3: 10.94 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:30:08.92 +55:07:45.3: 10.93 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 30 08.92 +55 07 45.3 10.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565050833867486464,2461258.6988,10.01,0.05,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
Gaia DR3 1565050833867486464 20260806.1988 10.01CV 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 08 06.1988 2461258.6988 9.91 13:35:28.25 +55:30:37.3
110.23970 60.51959 galactic UMa Second-epoch detections are separated by 0.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562165165598910208 | 13:35:28.26 +55:30:37.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.285+/-0.028 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:35:28.25 +55:30:37.3: 10.93 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:35:28.25 +55:30:37.3: 10.90 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.91 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 35 28.25 +55 30 37.3 9.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562165165598910208,2461258.6988,9.91,0.05,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
Gaia DR3 1562165165598910208 20260806.1988 9.91CV 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 08 06.1988 2461258.6988 9.84 13:29:42.05 +57:05:43.8
112.75617 59.27042 galactic UMa Second-epoch detections are separated by 0.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565694048169224576 | 13:29:42.04 +57:05:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.252+/-0.029 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:29:42.05 +57:05:43.8: 10.83 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:29:42.05 +57:05:43.8: 10.83 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 29 42.05 +57 05 43.8 9.8 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
Gaia DR3 1565694048169224576,2461258.6988,9.84,0.05,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 1565694048169224576 20260806.1988 9.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 9.79 13:26:36.20 +57:53:55.1
113.96016 58.61288 galactic UMa Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566058089596879360 | 13:26:36.25 +57:53:54.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5) J-Ks=0.284+/-0.028 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:26:36.20 +57:53:55.1: 10.77 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:26:36.20 +57:53:55.1: 10.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.77 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 26 36.20 +57 53 55.1 9.8 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
Gaia DR3 1566058089596879360,2461258.6988,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1566058089596879360 20260806.1988 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 9.57 13:35:11.81 +54:56:50.8
109.91429 61.06106 galactic UMa Second-epoch detections are separated by 0.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562124655469324416 | 13:35:11.81 +54:56:50.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.472+/-0.030 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:35:11.81 +54:56:50.8: 10.53 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:35:11.81 +54:56:50.8: 10.49 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.51 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 35 11.81 +54 56 50.8 9.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562124655469324416,2461258.6988,9.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1562124655469324416 20260806.1988 9.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 9.55 13:26:09.81 +58:11:20.2
114.21129 58.34749 galactic UMa Second-epoch detections are separated by 0.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566071318096161408 | 13:26:09.78 +58:11:20.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.265+/-0.032 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:26:09.81 +58:11:20.2: 10.53 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:26:09.81 +58:11:20.2: 10.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.52 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 26 09.81 +58 11 20.2 9.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566071318096161408,2461258.6988,9.55,0.05,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 1566071318096161408 20260806.1988 9.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 9.36 13:37:43.90 +57:49:36.4
111.22316 58.23672 galactic UMa Second-epoch detections are separated by 0.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1661843316360830592 | 13:37:43.95 +57:49:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.600+/-0.038 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:37:43.90 +57:49:36.4: 10.30 +/- 0.00 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:37:43.90 +57:49:36.4: 10.30 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.30 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 37 43.90 +57 49 36.4 9.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1661843316360830592,2461258.6988,9.36,0.05,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 1661843316360830592 20260806.1988 9.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.69 13:35:02.96 +55:22:48.2
110.26257 60.66251 galactic UMa Second-epoch detections are separated by 0.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562158018774765568 | 13:35:03.10 +55:22:48.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.510+/-0.037 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:35:02.96 +55:22:48.2: 11.88 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:35:02.96 +55:22:48.2: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 35 02.96 +55 22 48.2 10.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562158018774765568,2461258.6988,10.69,0.05,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
Gaia DR3 1562158018774765568 20260806.1988 10.69CV 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 08 06.1988 2461258.6988 10.77 13:32:30.14 +55:07:47.4
110.79193 61.01998 galactic UMa Second-epoch detections are separated by 0.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562138777321241088 | 13:32:30.17 +55:07:47.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.775+/-0.036 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:32:30.14 +55:07:47.4: 11.84 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:32:30.14 +55:07:47.4: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 32 30.14 +55 07 47.4 10.8 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
Gaia DR3 1562138777321241088,2461258.6988,10.77,0.05,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 1562138777321241088 20260806.1988 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.61 13:34:18.21 +56:21:11.8
111.11979 59.78109 galactic UMa Second-epoch detections are separated by 0.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J203.5761+56.3532 | 13:34:18.26 +56:21:11.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.333+/-0.027 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:34:18.21 +56:21:11.8: 11.83 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:34:18.21 +56:21:11.8: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 34 18.21 +56 21 11.8 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J203.5761+56.3532,2461258.6988,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J203.5761+56.3532 20260806.1988 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.61 13:34:48.59 +57:26:06.3
111.68121 58.73575 galactic UMa Second-epoch detections are separated by 0.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565762797713595264 | 13:34:48.56 +57:26:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.407+/-0.027 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:34:48.59 +57:26:06.3: 11.81 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:34:48.59 +57:26:06.3: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 34 48.59 +57 26 06.3 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565762797713595264,2461258.6988,10.61,0.05,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 1565762797713595264 20260806.1988 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.69 13:27:17.06 +56:28:03.0
113.03209 59.96644 galactic UMa Second-epoch detections are separated by 0.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565461467100353408 | 13:27:17.07 +56:28:02.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.337+/-0.028 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:27:17.06 +56:28:03.0: 11.79 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:27:17.06 +56:28:03.0: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 27 17.06 +56 28 03.0 10.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565461467100353408,2461258.6988,10.69,0.05,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
Gaia DR3 1565461467100353408 20260806.1988 10.69CV 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 08 06.1988 2461258.6988 10.60 13:30:51.98 +57:50:11.6
112.88274 58.51581 galactic UMa Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566021629618698624 | 13:30:52.05 +57:50:11.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.377+/-0.025 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:30:51.98 +57:50:11.6: 11.79 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:30:51.98 +57:50:11.6: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 30 51.98 +57 50 11.6 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566021629618698624,2461258.6988,10.60,0.05,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 1566021629618698624 20260806.1988 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.64 13:28:37.91 +56:47:39.1
112.86084 59.60088 galactic UMa Second-epoch detections are separated by 0.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565660444345089664 | 13:28:37.89 +56:47:38.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.328+/-0.032 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:28:37.91 +56:47:39.1: 11.79 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:28:37.91 +56:47:39.1: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 28 37.91 +56 47 39.1 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565660444345089664,2461258.6988,10.64,0.05,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 1565660444345089664 20260806.1988 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.62 13:25:34.74 +57:55:45.3
114.22769 58.61831 galactic UMa Second-epoch detections are separated by 0.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565968135802113664 | 13:25:34.73 +57:55:44.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.231+/-0.026 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:25:34.74 +57:55:45.3: 11.78 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:25:34.74 +57:55:45.3: 11.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 25 34.74 +57 55 45.3 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565968135802113664,2461258.6988,10.62,0.05,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
Gaia DR3 1565968135802113664 20260806.1988 10.62CV 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 08 06.1988 2461258.6988 10.64 13:28:25.05 +55:52:20.8
112.38756 60.49232 galactic UMa Second-epoch detections are separated by 0.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565226446490261760 | 13:28:25.11 +55:52:20.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.507+/-0.031 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:28:25.05 +55:52:20.8: 11.76 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:28:25.05 +55:52:20.8: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 28 25.05 +55 52 20.8 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565226446490261760,2461258.6988,10.64,0.05,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 1565226446490261760 20260806.1988 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.57 13:27:59.57 +56:11:43.2
112.68993 60.20010 galactic UMa Second-epoch detections are separated by 0.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565266303786808064 | 13:27:59.62 +56:11:43.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.475+/-0.033 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:27:59.57 +56:11:43.2: 11.74 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:27:59.57 +56:11:43.2: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 27 59.57 +56 11 43.2 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565266303786808064,2461258.6988,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565266303786808064 20260806.1988 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.58 13:36:11.79 +55:41:07.1
110.16797 60.31995 galactic UMa Second-epoch detections are separated by 0.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562543157080522624 | 13:36:11.75 +55:41:06.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5) J-Ks=0.309+/-0.028 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:36:11.79 +55:41:07.1: 11.73 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:36:11.79 +55:41:07.1: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 36 11.79 +55 41 07.1 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562543157080522624,2461258.6988,10.58,0.05,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 1562543157080522624 20260806.1988 10.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.55 13:36:03.90 +55:45:03.5
110.24911 60.26483 galactic UMa Second-epoch detections are separated by 0.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562545046866140288 | 13:36:03.91 +55:45:04.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.581+/-0.030 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:36:03.90 +55:45:03.5: 11.70 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:36:03.90 +55:45:03.5: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 36 03.90 +55 45 03.5 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562545046866140288,2461258.6988,10.55,0.05,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 1562545046866140288 20260806.1988 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.58 13:28:32.27 +57:16:13.5
113.14849 59.14758 galactic UMa Second-epoch detections are separated by 0.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565887630935032576 | 13:28:32.29 +57:16:13.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.337+/-0.033 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:28:32.27 +57:16:13.5: 11.69 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:28:32.27 +57:16:13.5: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 28 32.27 +57 16 13.5 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565887630935032576,2461258.6988,10.58,0.05,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 1565887630935032576 20260806.1988 10.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.61 13:29:31.13 +54:38:43.4
111.31774 61.61584 galactic UMa Second-epoch detections are separated by 0.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565008433950304640 | 13:29:31.14 +54:38:43.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A8III (LAMOST DR5) J-Ks=0.221+/-0.030 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:29:31.13 +54:38:43.4: 11.68 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:29:31.13 +54:38:43.4: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 29 31.13 +54 38 43.4 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565008433950304640,2461258.6988,10.61,0.05,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 1565008433950304640 20260806.1988 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.57 13:25:31.18 +57:34:57.9
114.07218 58.95541 galactic UMa Second-epoch detections are separated by 0.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565954421970888064 | 13:25:31.19 +57:34:58.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.600+/-0.029 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:25:31.18 +57:34:57.9: 11.68 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:25:31.18 +57:34:57.9: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 25 31.18 +57 34 57.9 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565954421970888064,2461258.6988,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565954421970888064 20260806.1988 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.60 13:27:09.74 +55:21:59.7
112.43696 61.02778 galactic UMa Second-epoch detections are separated by 0.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565114120209635456 | 13:27:09.87 +55:22:00.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:27:09.74 +55:21:59.7: 11.64 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:27:09.74 +55:21:59.7: 11.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 27 09.74 +55 21 59.7 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565114120209635456,2461258.6988,10.60,0.05,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 1565114120209635456 20260806.1988 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.65 13:19:57.09 +57:14:25.4
115.33706 59.46543 galactic UMa Second-epoch detections are separated by 0.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566308125413376128 | 13:19:57.11 +57:14:25.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.394+/-0.028 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:19:57.09 +57:14:25.4: 11.64 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:19:57.09 +57:14:25.4: 11.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 19 57.09 +57 14 25.4 10.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566308125413376128,2461258.6988,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1566308125413376128 20260806.1988 10.65CV 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 08 06.1988 2461258.6988 10.53 13:27:58.43 +56:06:08.1
112.64164 60.29008 galactic UMa Second-epoch detections are separated by 0.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565242320689424768 | 13:27:58.45 +56:06:08.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.599+/-0.032 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:27:58.43 +56:06:08.1: 11.62 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:27:58.43 +56:06:08.1: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 27 58.43 +56 06 08.1 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565242320689424768,2461258.6988,10.53,0.05,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 1565242320689424768 20260806.1988 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.54 13:33:15.68 +55:22:25.9
110.74702 60.75395 galactic UMa Second-epoch detections are separated by 0.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1562149188322027520 | 13:33:15.64 +55:22:26.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.355+/-0.033 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:33:15.68 +55:22:25.9: 11.61 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:33:15.68 +55:22:25.9: 11.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 33 15.68 +55 22 25.9 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1562149188322027520,2461258.6988,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1562149188322027520 20260806.1988 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.46 13:34:38.85 +57:20:06.3
111.65893 58.83746 galactic UMa Second-epoch detections are separated by 0.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565762011731450496 | 13:34:38.82 +57:20:05.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.268+/-0.027 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:34:38.85 +57:20:06.3: 11.61 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:34:38.85 +57:20:06.3: 11.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 34 38.85 +57 20 06.3 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565762011731450496,2461258.6988,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565762011731450496 20260806.1988 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.51 13:17:19.63 +57:39:02.2
116.17959 59.13694 galactic UMa Second-epoch detections are separated by 0.1" and 8.2 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 | ATO J199.3328+57.6506 | 13:17:19.85 +57:39:02.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M1 2014MNRAS.443.2561G 2MASS J13172018+5739010
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:17:19.63 +57:39:02.2: 11.59 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:17:19.63 +57:39:02.2: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 17 19.63 +57 39 02.2 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J199.3328+57.6506,2461258.6988,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J199.3328+57.6506 20260806.1988 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.56 13:27:32.49 +54:55:50.9
112.06791 61.42938 galactic UMa Second-epoch detections are separated by 0.3" and 8.4 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 1565080039645130752 | 13:27:32.47 +54:55:50.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F9 (LAMOST DR5) J-Ks=0.381+/-0.036 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:27:32.49 +54:55:50.9: 11.58 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:27:32.49 +54:55:50.9: 11.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 27 32.49 +54 55 50.9 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1565080039645130752,2461258.6988,10.56,0.05,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 1565080039645130752 20260806.1988 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.62 13:13:07.06 +58:17:02.6
117.46087 58.61331 galactic UMa Second-epoch detections are separated by 0.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1566611624982195456 | 13:13:07.02 +58:17:02.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.285+/-0.027 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:13:07.06 +58:17:02.6: 11.58 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:13:07.06 +58:17:02.6: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 13 07.06 +58 17 02.6 10.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1566611624982195456,2461258.6988,10.62,0.05,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
Gaia DR3 1566611624982195456 20260806.1988 10.62CV 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 08 06.1988 2461258.6988 10.44 13:33:02.67 +58:01:04.6
112.45962 58.25636 galactic UMa Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565840558093415424 | 13:33:02.60 +58:01:04.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1956PMcCO..13a....B AG+58 895 J-Ks=0.324+/-0.030 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:33:02.67 +58:01:04.6: 11.57 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:33:02.67 +58:01:04.6: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 33 02.67 +58 01 04.6 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565840558093415424,2461258.6988,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565840558093415424 20260806.1988 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.40 13:32:21.75 +56:49:55.0
111.92244 59.41298 galactic UMa Second-epoch detections are separated by 0.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565672367174239872 | 13:32:21.71 +56:49:54.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.380+/-0.038 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:32:21.75 +56:49:55.0: 11.57 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:32:21.75 +56:49:55.0: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 32 21.75 +56 49 55.0 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565672367174239872,2461258.6988,10.40,0.05,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 1565672367174239872 20260806.1988 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.54 13:28:12.62 +55:29:03.5
112.21379 60.87215 galactic UMa Second-epoch detections are separated by 0.6" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565118793133378688 | 13:28:12.60 +55:29:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.384+/-0.029 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:28:12.62 +55:29:03.5: 11.57 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:28:12.62 +55:29:03.5: 11.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 28 12.62 +55 29 03.5 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565118793133378688,2461258.6988,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565118793133378688 20260806.1988 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.42 13:33:14.41 +56:51:02.5
111.71022 59.35753 galactic UMa Second-epoch detections are separated by 0.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565630791890815488 | 13:33:14.43 +56:51:02.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.680+/-0.028 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:33:14.41 +56:51:02.5: 11.55 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:33:14.41 +56:51:02.5: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 33 14.41 +56 51 02.5 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565630791890815488,2461258.6988,10.42,0.05,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 1565630791890815488 20260806.1988 10.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.43 13:30:10.43 +55:54:10.4
111.92917 60.39020 galactic UMa Second-epoch detections are separated by 0.3" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565200401808580224 | 13:30:10.49 +55:54:10.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M2 (LAMOST DR5) J-Ks=0.820+/-0.030 (M)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:30:10.43 +55:54:10.4: 11.55 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:30:10.43 +55:54:10.4: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 30 10.43 +55 54 10.4 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565200401808580224,2461258.6988,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565200401808580224 20260806.1988 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.37 13:29:09.05 +57:22:17.2
113.04930 59.02735 galactic UMa Second-epoch detections are separated by 0.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565891376146517632 | 13:29:08.98 +57:22:17.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.300+/-0.030 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:29:09.05 +57:22:17.2: 11.47 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:29:09.05 +57:22:17.2: 11.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 29 09.05 +57 22 17.2 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565891376146517632,2461258.6988,10.37,0.05,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 1565891376146517632 20260806.1988 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.46 13:27:38.84 +54:49:37.0
111.97374 61.52423 galactic UMa Second-epoch detections are separated by 0.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565026369732298240 | 13:27:38.86 +54:49:37.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.560+/-0.031 (K)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:27:38.84 +54:49:37.0: 11.46 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:27:38.84 +54:49:37.0: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 27 38.84 +54 49 37.0 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565026369732298240,2461258.6988,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565026369732298240 20260806.1988 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.30 13:28:49.36 +57:05:53.9
112.98146 59.30188 galactic UMa Second-epoch detections are separated by 0.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565880930786047872 | 13:28:49.42 +57:05:54.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5) J-Ks=0.956+/-0.030 (M)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:28:49.36 +57:05:53.9: 11.45 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:28:49.36 +57:05:53.9: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 28 49.36 +57 05 53.9 10.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565880930786047872,2461258.6988,10.30,0.05,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 1565880930786047872 20260806.1988 10.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.43 13:26:36.05 +55:46:30.0
112.82918 60.65820 galactic UMa Second-epoch detections are separated by 0.1" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565140066108109568 | 13:26:36.05 +55:46:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.272+/-0.031 (F)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:26:36.05 +55:46:30.0: 11.46 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:26:36.05 +55:46:30.0: 11.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 26 36.05 +55 46 30.0 10.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565140066108109568,2461258.6988,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565140066108109568 20260806.1988 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.1988 2461258.6988 10.54 13:26:09.73 +55:23:20.2
112.73147 61.04629 galactic UMa Second-epoch detections are separated by 0.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1565125222701138816 | 13:26:09.76 +55:23:20.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.352+/-0.033 (G)
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits at 13:26:09.73 +55:23:20.2: 11.45 +/- 0.01 detection
Forced photometry on wcs_UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits at 13:26:09.73 +55:23:20.2: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.1988* 13 26 09.73 +55 23 20.2 10.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1565125222701138816,2461258.6988,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1565125222701138816 20260806.1988 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.78072922 22.02.2026 06:44:05.005 /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits
First image: 2461093.78072922 22.02.2026 06:44:05.005 /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits
Last image: 2461258.69907061 06.08.2026 04:46:29.701 /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 148
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 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): 6140
Objects passed selection criteria: 6103
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 3893.5
Average stars matched: 3781.75 (97.1298 %)
Memory usage VmPeak: 232576 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 5 23:50:55 CDT 2026
Host name: tau
############################################################
WARNING: VaST exited with code 1 on the field UMa-08-Q1b1x1 after completing the measurements (memory cleanup crash); the transient search continues.
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 2
Ref. image: 2461093.78072922 22.02.2026 06:44:05.005 /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits
First image: 2461093.78072922 22.02.2026 06:44:05.005 /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits
Last image: 2461093.78148399 22.02.2026 06:45:10.217 /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 9 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): 29570
Objects passed selection criteria: 29412
Measurements per detected object (mean, median, min, max): 2.0 2.0 2 2
Measurements per selected object (mean, median, min, max): 2.0 2.0 2 2
Average stars detected per image: 31769.5
Average stars matched: 30682 (96.5769 %)
Memory usage VmPeak: 253740 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 5 23:56:10 CDT 2026
Host name: tau
***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
############################################################
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Considering the candidate 03486_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
The candidate 03486_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 11:53:50.25 +53:41:43.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 03411_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
The candidate 03411_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 13:23:55.73 +54:55:30.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 03975_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
The candidate 03975_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 12:54:01.79 +55:57:35.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 03458_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03458_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03541_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03541_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04587_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04587_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05200_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05200_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04908_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04908_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05302_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05302_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04458_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04458_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05154_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05154_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04602_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04602_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04168_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04168_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03993_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03993_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04954_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04954_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03399_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03399_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03227_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03227_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04400_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04400_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 02563_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 02563_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03257_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03257_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05092_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05092_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05152_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05152_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05036_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05036_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03969_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03969_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04557_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04557_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04365_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04365_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05096_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05096_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04614_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04614_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05136_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05136_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03690_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03690_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04851_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04851_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04510_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04510_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05812_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05812_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05632_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05632_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05172_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05172_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04599_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04599_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04481_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04481_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04140_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04140_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04913_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04913_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05794_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05794_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04202_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04202_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04322_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04322_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05725_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05725_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04114_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04114_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05730_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05730_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03668_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03668_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03268_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03268_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04976_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04976_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03919_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03919_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04789_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04789_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 02950_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 02950_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05536_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05536_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05104_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05104_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05010_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05010_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04246_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04246_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04837_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04837_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05809_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05809_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04668_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04668_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03886_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03886_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05872_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05872_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04330_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04330_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04664_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04664_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04454_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04454_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04605_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04605_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04751_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04751_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05535_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05535_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03984_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03984_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03317_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03317_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04035_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04035_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05918_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05918_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04966_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04966_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04815_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04815_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03551_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03551_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05658_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05658_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05181_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05181_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04022_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04022_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05681_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05681_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03104_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03104_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04524_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04524_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 02897_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 02897_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04355_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04355_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03298_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03298_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04859_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04859_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03296_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03296_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04222_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04222_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05889_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05889_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04758_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04758_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04240_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04240_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03687_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03687_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03944_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03944_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04865_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04865_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04973_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
The candidate 04973_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 13:27:33.43 +57:16:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05824_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05824_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03620_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03620_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05380_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05380_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05766_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05766_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03869_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03869_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03701_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03701_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04467_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04467_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05142_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05142_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04484_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04484_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05887_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05887_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04688_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04688_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05391_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05391_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04108_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04108_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04315_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04315_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04057_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04057_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04096_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04096_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04981_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04981_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03402_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03402_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05167_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05167_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03799_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03799_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04911_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04911_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04247_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04247_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03851_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03851_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05068_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05068_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05170_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05170_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03548_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03548_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05596_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05596_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05733_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05733_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04736_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04736_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03876_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03876_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04759_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04759_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04135_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04135_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 05040_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 05040_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03488_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03488_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04866_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04866_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 04036_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 04036_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 03808_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 03808_fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119
make_report_in_HTML.sh Phase 2 (HTML assembly): 9s
make_report_in_HTML.sh TOTAL: 245s
Prepared the HTML report for the field UMa-08-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 ####
13:34:27.04 +53:08:32.6
13:31:59.09 +53:43:16.7
13:34:02.26 +53:45:49.8
13:30:04.64 +54:05:47.9
13:34:29.99 +54:15:13.6
13:29:45.28 +54:22:32.6
13:35:00.05 +54:19:57.5
13:29:41.46 +54:26:58.1
13:31:49.34 +54:25:39.5
13:29:31.07 +54:28:48.1
13:34:20.56 +54:34:42.8
13:29:31.13 +54:38:43.4
13:34:41.89 +54:41:13.1
13:27:38.84 +54:49:37.0
13:25:55.53 +54:55:18.2
13:27:32.49 +54:55:50.9
13:28:57.34 +54:55:28.8
13:35:11.81 +54:56:50.8
13:34:38.50 +55:02:23.1
13:30:08.92 +55:07:45.3
13:33:46.98 +55:05:27.0
13:32:30.14 +55:07:47.4
13:27:09.74 +55:21:59.7
13:26:09.73 +55:23:20.2
13:33:15.68 +55:22:25.9
13:35:02.96 +55:22:48.2
13:28:12.62 +55:29:03.5
13:26:27.45 +55:31:27.0
13:30:06.85 +55:32:44.9
13:35:28.25 +55:30:37.3
13:36:04.83 +55:33:13.9
13:24:35.97 +55:42:48.2
13:24:40.14 +55:43:16.2
13:32:12.43 +55:41:13.6
13:35:42.07 +55:39:46.8
13:26:36.05 +55:46:30.0
13:36:11.79 +55:41:07.1
13:36:03.90 +55:45:03.5
13:28:25.05 +55:52:20.8
13:24:10.58 +55:55:38.0
13:30:10.43 +55:54:10.4
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13:25:06.01 +56:03:55.8
13:35:29.99 +55:58:19.5
13:33:05.99 +56:01:54.6
13:33:16.68 +56:02:20.7
13:27:58.43 +56:06:08.1
13:27:59.57 +56:11:43.2
13:30:45.23 +56:10:21.4
13:20:40.79 +56:16:55.4
13:26:52.16 +56:17:06.8
13:31:13.88 +56:14:46.3
13:23:16.05 +56:22:41.7
13:32:39.41 +56:21:47.7
13:33:48.65 +56:21:08.6
13:34:18.21 +56:21:11.8
13:30:35.53 +56:25:59.8
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13:30:19.90 +56:33:19.9
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13:31:38.23 +57:46:45.5
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-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-45-36_20.00sec_0.00C_LIGHTs_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits
Last image: 2461258.69845010 06.08.2026 04:45:36.089 UTC
WARNING: VaST exited with code 1 on the field UMa-08-Q1b1x1 AFTER completing the measurements. This is a memory-management crash during cleanup (a VaST bug to report), NOT a wrong field / clouds / bad focus. The lightcurves were written, so the transient search continues.
____ VaST output (crashed during memory cleanup; the measurements above are complete) ____
--==VaST 1.0rc90==--
Parsing command line arguments...
opt 'F': Will NOT create flag images for SExtractor
opt '5': 5.000000 pix is the new fixed star matching radius!
opt 'b': Using 500 reference stars for image matching!
opt '3': Will try to select best aperture for each source!
opt 'y': 0 SysRem iterations will be conducted!
opt 't 4': robust linear magnitude calibration (vary zero-point and slope)
opt 'x': 99 is the maximum acceptable SExtractor flag!
WARNING: disabling the mag-size filter in order not to reject blended stars.
opt 'u': Stick with UTC time system, no conversion to TT will be done!
opt 'f': Run ./find_candidates manually!
opt 'k': "JD" keyword in FITS image header will be ignored!
INFO from vast_remove_directory(): Could not open directory: symlinks_to_images
INFO from vast_remove_directory(): Could not open directory: converted_images
INFO from vast_remove_directory(): Could not open directory: unpacked_images
Checking the list of input images specified on the command line ...
Looking for the list of input images with time corrections in vast_list_of_input_images_with_time_corrections.txt ... list not found.
This is OK if you specify the input images on the command line, not through this text file.
Checking write permissions for the current directory (/data_ssd/NMW-TexasTech/workdir/vast_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt)... OK
Found a system-wide installation of SExtractor
Cleaning old outNNNNN.dat files.
Done with cleaning!
VaST was started with the following command line:
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-45-36_20.00sec_0.00C_LIGHTs_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits
Preparing to process 4 input FITS images...
######## Forcing special settings for the transient detection ########
transient search mode: disabling the mag-size filter as it should be switched off when running a transient search!
transient search mode: disabling the bad image filter as it will not help during the transient search!
transient search mode: will not try to gues image saturation limit
transient search mode: no UTC-to-TT time system conversion will be performed!!!
transient search mode: setting the maximum acceptable SExtractor flag to 3
transient search mode: disabling rejectin of images with elliptical stars
transient search mode: not discarding large sources
################
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).
Setting the fixed star match radius of 5.00 pix
We have 4 images to process.
SExtractor catalog cache: restored UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits catalog from cache
SExtractor catalog cache: restored UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits catalog from cache
Running SExtractor in 3 parallel threads...
Using the catalog image00001.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits
Using the catalog image00002.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits
The gain value (GAIN=0.830) from default.sex will be used for image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-45-36_20.00sec_0.00C_LIGHTs_0118.fits
The above guess is based on the non-default gain value specified in default.sex by user
Parent process says: we are done fork()ing.
Waiting for thread 2 to finish...
autodetect_aperture() is running SExtractor on /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-45-36_20.00sec_0.00C_LIGHTs_0118.fits
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).
autodetect_aperture() is doing a preliminary SExtractor run to determine an appropriate aperture size
sex -c default.sex -PARAMETERS_NAME autodetect_aper.param -CATALOG_NAME autodetect_aper_image00003.cat /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-45-36_20.00sec_0.00C_LIGHTs_0118.fits > image00003.cat.sex_log 2>&1
The gain value (GAIN=0.830) from default.sex will be used for image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits
The above guess is based on the non-default gain value specified in default.sex by user
autodetect_aperture() is running SExtractor on /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits
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).
autodetect_aperture() is doing a preliminary SExtractor run to determine an appropriate aperture size
sex -c default.sex -PARAMETERS_NAME autodetect_aper.param -CATALOG_NAME autodetect_aper_image00004.cat /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits > image00004.cat.sex_log 2>&1
autodetect_aperture() is doing the main SExtractor run
sex -PARAMETERS_NAME default.param -PHOT_APERTURES 5.5,5.5,4.9,6.0,6.5,7.1 -VERBOSE_TYPE NORMAL -CATALOG_NAME image00004.cat /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits > image00004.cat.sex_log 2>&1
autodetect_aperture() is doing the main SExtractor run
sex -PARAMETERS_NAME default.param -PHOT_APERTURES 5.5,5.5,5.0,6.1,6.6,7.2 -VERBOSE_TYPE NORMAL -CATALOG_NAME image00003.cat /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-45-36_20.00sec_0.00C_LIGHTs_0118.fits > image00003.cat.sex_log 2>&1
autodetect_aperture() is done with image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits
Waiting for thread 1 to finish...
autodetect_aperture() is done with image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-45-36_20.00sec_0.00C_LIGHTs_0118.fits
Done with SExtractor!
TIMING SExtractor: 5 seconds
Matching stars between images!
No manually selected comparison stars file manually_selected_comparison_stars.lst which is fine.
Processing /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits
9576x6388 FITS image /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits
Trying to guess the time system by parsing the comment string 'Time of observation (UTC)'
Time system set from the comment to DATE-OBS keyword: 'Time of observation (UTC)'
The input time system is identified as: UTC (blank if unknown)
Setting observation date using DATE-OBS keyword: 2026-02-22T06:44:05.0056361
Setting observation time using DATE-OBS keyword: 2026-02-22T06:44:05.0056361
Observing time converted to the "standard" FITS header format:
DATE-OBS= 2026-02-22T06:44:05.005
EXPTIME = 20.000
Using the catalog image00001.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits
Exposure 20 sec, 22.02.2026 06:44:05.005 UTC = JD(UTC) 2461093.78072922 mid. exp.
The reference image star 8498.004 872.033 is rejected, see bad_region.lst
The reference image star 4000.998 1321.993 is rejected, see bad_region.lst
The reference image star 881.248 1380.213 is rejected, see bad_region.lst
The reference image star 3619.001 1437.160 is rejected, see bad_region.lst
The reference image star 351.992 1876.002 is rejected, see bad_region.lst
The reference image star 7039.016 5906.003 is rejected, see bad_region.lst
The reference image star 8216.956 3949.999 is rejected, see bad_region.lst
The reference image star 5376.997 4998.006 is rejected, see bad_region.lst
The reference image star 2318.002 4332.008 is rejected, see bad_region.lst
SExtractor output filtering results:
* passed selection: 31794, (31794 good for image matching)
* rejected as having no flux measurement: 0
* rejected as having SNR<3.0: 24
* rejected inside rectangles defined in bad_region.lst: 9
* rejected close to frame edge: 170
* rejected as being too small (<1.3 pix): 0
* rejected as being too large (>5.1 pix): 0
* rejected as outliers in mag-size plot: 0
* rejected as having SExtractor flags > 99 and <= 7: 0
* rejected as having hopelessly bad SExtractor flags (>7): 63
* rejected due to an external image flag: 0
* rejected as having bad PSF fit: 0
---
You may change some of the filtering parameters by editing src/vast_limits.h and re-running 'make'.
Please note: the CCD position-dependent magnitude correction will be applied.
get_detection_limit_sn(): Detection limit: -7.27
Detection limit from the magnitude-SNR relation= -7.3 (5.0 sigma detection)
The simple faintest star detection limit= -6.6
80 percent brightest stars detection limit= -7.8
Selected detection limit= -7.8
Final detection limit= -7.8 (after subtracting MAG_TRANSIENT_ABOVE_THE_REFERENCE_FRAME_LIMIT=0.0)
Parameter box for transient search: 10.05.1 pix): 0
* rejected as outliers in mag-size plot: 0
* rejected as having SExtractor flags > 99 and <= 7: 0
* rejected as having hopelessly bad SExtractor flags (>7): 67
* rejected due to an external image flag: 0
* rejected as having bad PSF fit: 0
---
You may change some of the filtering parameters by editing src/vast_limits.h and re-running 'make'.
31745 * detected, using 499/ 500 * for reference/current image matching, fraction_of_ambiguous_matches= 0.011417, number_of_ambiguous_matches=363
refining the coordinate transformation... [CVPOLY iter 1: order=1 pairs=29647 inliers=29647 rms 0.44 -> 0.43 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.009562, number_of_ambiguous_matches=304
29644 * matched, [CVPOLY iter 2: order=1 pairs=29644 inliers=29644 rms 0.42 -> 0.42 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.005347, number_of_ambiguous_matches=170
29634 * matched (2nd iteration). [CVPOLY iter 3: order=1 pairs=29634 inliers=29634 rms 0.36 -> 0.36 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.002139, number_of_ambiguous_matches=68
29570 * matched (3rd iteration). Success!
rotation [degrees] = 0.010
31745 stars detected, 29570 stars matched
Performing magnitude calibration using automatically selected comparison stars
Expecting to find at least 40 * for magnitude calibration
We have N_good_stars = 28280, N_manually_selected_comparison_stars = 0
Using 28280 stars for magnitude calibration (before filtering).
Iteratively removing outliers from the linear mag-mag relation (unweighted fit)...
After removing outliers in (X,Y,dm) plane, we are left with 28278 stars for magnitude calibration.
Using the linear CCD position-dependent magnitude correction:
delta_m = 0.00000*X_pix -0.00000*Y_pix -0.00044
Iteratively removing outliers from the mag-mag relation (weighted linear/polynomial fit)...
Computing robust linear magnitude calibration.
Used 26875 stars for magnitude calibration (after filtering).
get_detection_limit_sn(): Detection limit: -7.27
33969 objects stored in memory (1000000 max.)
Magnitude calibration is performed successfully!
Saving observations to the cache... OK
memory: 214032 kB used, 253740 kB peak, 65263848 kB available RAM
processed 2 of 4 images ( 50.0%)
Processing /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-45-36_20.00sec_0.00C_LIGHTs_0118.fits
9576x6388 FITS image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-45-36_20.00sec_0.00C_LIGHTs_0118.fits
Trying to guess the time system by parsing the comment string 'Time of observation (UTC)'
Time system set from the comment to DATE-OBS keyword: 'Time of observation (UTC)'
The input time system is identified as: UTC (blank if unknown)
Setting observation date using DATE-OBS keyword: 2026-08-06T04:45:36.0896993
Setting observation time using DATE-OBS keyword: 2026-08-06T04:45:36.0896993
Observing time converted to the "standard" FITS header format:
DATE-OBS= 2026-08-06T04:45:36.089
EXPTIME = 20.000
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-45-36_20.00sec_0.00C_LIGHTs_0118.fits
The star 1158.093 135.990 is rejected, see bad_region.lst
The star 8498.000 872.012 is rejected, see bad_region.lst
The star 1152.048 919.007 is rejected, see bad_region.lst
The star 191.061 1040.052 is rejected, see bad_region.lst
The star 1201.304 1170.829 is rejected, see bad_region.lst
The star 3619.003 1436.993 is rejected, see bad_region.lst
The star 351.999 1875.993 is rejected, see bad_region.lst
The star 4923.001 2428.061 is rejected, see bad_region.lst
The star 1454.946 3132.999 is rejected, see bad_region.lst
The star 5282.009 5086.004 is rejected, see bad_region.lst
Excluding more stars falling at bad regions!.. (will not print them all)
SExtractor output filtering results:
* passed selection: 8797
* rejected as having no flux measurement: 0
* rejected as having SNR<3.0: 1
* rejected inside rectangles defined in bad_region.lst: 13
* rejected close to frame edge: 62
* rejected as being too small (<1.4 pix): 0
* rejected as being too large (>5.5 pix): 0
* rejected as outliers in mag-size plot: 0
* rejected as having SExtractor flags > 99 and <= 7: 0
* rejected as having hopelessly bad SExtractor flags (>7): 68
* rejected due to an external image flag: 0
* rejected as having bad PSF fit: 0
---
You may change some of the filtering parameters by editing src/vast_limits.h and re-running 'make'.
8797 * detected, using 138/ 500 * for reference/current image matching, fraction_of_ambiguous_matches= 0.000383, number_of_ambiguous_matches=13
refining the coordinate transformation... [CVPOLY iter 1: order=3 pairs=8013 inliers=8013 rms 1.49 -> 0.29 pix, max corner correction 4.4 pix] fraction_of_ambiguous_matches= 0.000324, number_of_ambiguous_matches=11
8015 * matched, [CVPOLY iter 2: order=1 pairs=8015 inliers=8015 rms 0.29 -> 0.29 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.000236, number_of_ambiguous_matches=8
8012 * matched (2nd iteration). [CVPOLY iter 3: order=1 pairs=8012 inliers=8012 rms 0.24 -> 0.24 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.000177, number_of_ambiguous_matches=6
8012 * matched (3rd iteration). Success!
rotation [degrees] = 171.427
8797 stars detected, 8012 stars matched
Performing magnitude calibration using automatically selected comparison stars
Expecting to find at least 40 * for magnitude calibration
We have N_good_stars = 7355, N_manually_selected_comparison_stars = 0
Using 7355 stars for magnitude calibration (before filtering).
Iteratively removing outliers from the linear mag-mag relation (unweighted fit)...
After removing outliers in (X,Y,dm) plane, we are left with 6019 stars for magnitude calibration.
Using the linear CCD position-dependent magnitude correction:
delta_m = 0.00016*X_pix +0.00014*Y_pix -0.93790
ERROR in magnitude calibration: fabs(lin_mag_A * X_im_size + lin_mag_B * Y_im_size + lin_mag_C) > MAX_LIN_CORR_MAG
Used 6019 stars for magnitude calibration (after filtering).
get_detection_limit_sn(): Detection limit: -7.64
[01;31m ERROR!!! Magnitude calibration failure. Dropping image. [33;00m
33969 objects stored in memory (1000000 max.)
memory: 214020 kB used, 253740 kB peak, 65263848 kB available RAM
processed 3 of 4 images ( 75.0%)
Processing /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits
9576x6388 FITS image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits
Trying to guess the time system by parsing the comment string 'Time of observation (UTC)'
Time system set from the comment to DATE-OBS keyword: 'Time of observation (UTC)'
The input time system is identified as: UTC (blank if unknown)
Setting observation date using DATE-OBS keyword: 2026-08-06T04:46:29.7018679
Setting observation time using DATE-OBS keyword: 2026-08-06T04:46:29.7018679
Observing time converted to the "standard" FITS header format:
DATE-OBS= 2026-08-06T04:46:29.701
EXPTIME = 20.000
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits
The star 8498.022 872.056 is rejected, see bad_region.lst
The star 1152.005 919.037 is rejected, see bad_region.lst
The star 191.096 1039.834 is rejected, see bad_region.lst
The star 883.660 1376.993 is rejected, see bad_region.lst
The star 3618.996 1437.001 is rejected, see bad_region.lst
The star 352.006 1876.009 is rejected, see bad_region.lst
The star 2636.129 2107.990 is rejected, see bad_region.lst
The star 4922.743 2427.801 is rejected, see bad_region.lst
The star 725.026 2731.454 is rejected, see bad_region.lst
The star 1455.000 3132.995 is rejected, see bad_region.lst
Excluding more stars falling at bad regions!.. (will not print them all)
SExtractor output filtering results:
* passed selection: 8298
* rejected as having no flux measurement: 0
* rejected as having SNR<3.0: 5
* rejected inside rectangles defined in bad_region.lst: 17
* rejected close to frame edge: 53
* rejected as being too small (<1.4 pix): 0
* rejected as being too large (>5.5 pix): 0
* rejected as outliers in mag-size plot: 0
* rejected as having SExtractor flags > 99 and <= 7: 0
* rejected as having hopelessly bad SExtractor flags (>7): 8
* rejected due to an external image flag: 0
* rejected as having bad PSF fit: 0
---
You may change some of the filtering parameters by editing src/vast_limits.h and re-running 'make'.
8298 * detected, using 130/ 500 * for reference/current image matching, fraction_of_ambiguous_matches= 0.000265, number_of_ambiguous_matches=9
refining the coordinate transformation... [CVPOLY iter 1: order=3 pairs=7558 inliers=7558 rms 1.28 -> 0.36 pix, max corner correction 2.3 pix] fraction_of_ambiguous_matches= 0.000265, number_of_ambiguous_matches=9
7557 * matched, [CVPOLY iter 2: order=1 pairs=7557 inliers=7557 rms 0.32 -> 0.32 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.000147, number_of_ambiguous_matches=5
7554 * matched (2nd iteration). [CVPOLY iter 3: order=1 pairs=7554 inliers=7554 rms 0.24 -> 0.24 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.000088, number_of_ambiguous_matches=3
7553 * matched (3rd iteration). Success!
rotation [degrees] = 171.403
8298 stars detected, 7553 stars matched
Performing magnitude calibration using automatically selected comparison stars
Expecting to find at least 40 * for magnitude calibration
We have N_good_stars = 6902, N_manually_selected_comparison_stars = 0
Using 6902 stars for magnitude calibration (before filtering).
Iteratively removing outliers from the linear mag-mag relation (unweighted fit)...
After removing outliers in (X,Y,dm) plane, we are left with 5911 stars for magnitude calibration.
Using the linear CCD position-dependent magnitude correction:
delta_m = 0.00014*X_pix +0.00011*Y_pix -0.85101
ERROR in magnitude calibration: fabs(lin_mag_A * X_im_size + lin_mag_B * Y_im_size + lin_mag_C) > MAX_LIN_CORR_MAG
Used 5911 stars for magnitude calibration (after filtering).
get_detection_limit_sn(): Detection limit: -7.65
[01;31m ERROR!!! Magnitude calibration failure. Dropping image. [33;00m
33969 objects stored in memory (1000000 max.)
memory: 214020 kB used, 253740 kB peak, 65263848 kB available RAM
processed 4 of 4 images (100.0%)
TIMING matching_and_photometry: 1 seconds
Done with measurements! =)
Total number of measurements 63539 (63539 measurements stored in RAM)
Freeing up some memory... Sorting the measurements cached in memory...
Writing lightcurve (outNNNNN.dat) files...
TIMING lightcurve_write: 1 seconds
The lightcurve files have been written, freeing up more memory...
Creating vast_image_details.log ...
Writing summary file: vast_summary.log ... OK
Selecting the best aperture for each source
Aperture with index 0 (REFERENCE_APERTURE_DIAMETER +0.00*REFERENCE_APERTURE_DIAMETER) seems best for 5749 stars
Aperture with index 1 (REFERENCE_APERTURE_DIAMETER +0.00*REFERENCE_APERTURE_DIAMETER) seems best for 0 stars
Aperture with index 2 (REFERENCE_APERTURE_DIAMETER -0.10*REFERENCE_APERTURE_DIAMETER) seems best for 8207 stars
Aperture with index 3 (REFERENCE_APERTURE_DIAMETER +0.10*REFERENCE_APERTURE_DIAMETER) seems best for 4142 stars
Aperture with index 4 (REFERENCE_APERTURE_DIAMETER +0.20*REFERENCE_APERTURE_DIAMETER) seems best for 4193 stars
Aperture with index 5 (REFERENCE_APERTURE_DIAMETER +0.30*REFERENCE_APERTURE_DIAMETER) seems best for 7279 stars
done! =)
TIMING select_aperture: 2 seconds
Computing lightcurve statistics... Will not compute variability indexes for objects having <1 points in lightcurve
You may disable this by commenting out the line '#define DROP_LIGHTCURVES_WITH_SMALL_NUMBER_OF_POINTS_FROM_ALL_PLOTS' in src/vast_limits.h an re-compiling VaST with 'make'
Computing, please wait a bit
......................................................................................................................................................................................................................................................................................................
vast_lightcurve_statistics.log: 29412 objects, the longest string is 383 bytes.
Allocating memory for resorting the file.
----***** VaST processing WARNING *****----
You asked VaST to process 4 images, but only 1 were actually matched to the reference one.
Please investigate this!
**************************************************************
This error might be a bug, but it is far more likely that it is caused by
inappropriate input data. A few simple things to check in the diagnostic
messages printed above (or the vast*.log files):
* How many of the input images are matched?
* Does the number of detected stars on each image look reasonable?
* Do images have a sufficient overlap of at least about 20 percent?
You may run
./sextract_single_image /path/to/my/image/file.fit
to see how well VaST detects stars with the current SExtractor settings
(star detection settings can be changed in the default.sex configuration
file, see various examples in the VaST directory).
If you cannot identify the problem, please e-mail Kirill Sokolovsky
Please try to describe the problem in details and, if possible, attach vast_summary.log
file and a few example images. If the images are too big to be sent by e-mail, please
upload them through a web-form http://scan.sai.msu.ru/upload/
**************************************************************
Low percentage of matched images - we'll declare this an unsuccessful VaST run (exit code 1)
_____________________
SExtractor catalog cache: saved UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits.cat to cache
SExtractor catalog cache: saved UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.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-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-45-36_20.00sec_0.00C_LIGHTs_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits
Last image: 2461258.69845010 06.08.2026 04:45:36.089 UTC
ERROR running VaST on the field UMa-08-Q1b1x1 (less than 4 images processed)
exp_start= 22.02.2026 06:44:05.005 exp= 20.000 JD= 2461093.78072922 ap= 5.1 rotation= 0.000 *detected= 31794 *matched= 31794 status=OK /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-44-05_20.00sec_-15.00C_LIGHT_0290.fits
exp_start= 22.02.2026 06:45:10.217 exp= 20.000 JD= 2461093.78148399 ap= 5.1 rotation= 0.010 *detected= 31745 *matched= 29570 status=OK /data_ssd/NMW-TexasTech/reference_imgs/UMa-08-Q1b1x1_2026-02-22_00-45-10_20.00sec_-15.00C_LIGHT_0291.fits
exp_start= 06.08.2026 04:45:36.089 exp= 20.000 JD= 2461258.69845010 ap= 5.5 rotation= 171.427 *detected= 8797 *matched= 8012 status=ERROR /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-45-36_20.00sec_0.00C_LIGHTs_0118.fits
exp_start= 06.08.2026 04:46:29.701 exp= 20.000 JD= 2461258.69907061 ap= 5.5 rotation= 171.403 *detected= 8298 *matched= 7553 status=ERROR /data_ssd/NMW-TexasTech/workdir//img_2026-08-05_CI_UMa-08-Q1b1x1_234832_TTUQ1b1x1_1131470_QZJtqbLt/fd_UMa-08-Q1b1x1_2026-08-05_23-46-29_20.00sec_-0.00C_LIGHTs_0119.fits
########### Completed UMa-08-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 ####
13:34:41.89 +54:41:13.1
13:25:55.53 +54:55:18.2
13:30:14.92 +56:36:07.6
13:31:15.03 +57:33:48.2
13:26:02.28 +57:11:14.2
13:15:30.00 +58:34:02.4
13:33:48.65 +56:21:08.6
13:19:45.22 +57:36:44.1
13:27:59.91 +56:39:40.6
13:30:16.46 +55:57:24.3
13:24:40.14 +55:43:16.2
13:25:48.19 +57:15:25.8
13:34:20.56 +54:34:42.8
13:34:29.99 +54:15:13.6
13:23:16.05 +56:22:41.7
13:34:27.04 +53:08:32.6
13:29:45.28 +54:22:32.6
13:28:11.42 +57:27:17.9
13:17:30.73 +57:37:26.8
13:31:31.66 +57:20:57.0
13:36:04.83 +55:33:13.9
13:30:19.90 +56:33:19.9
13:31:13.88 +56:14:46.3
13:25:43.05 +57:29:37.5
13:36:16.05 +56:34:35.0
13:29:48.87 +57:29:40.5
13:33:46.98 +55:05:27.0
13:22:49.06 +57:08:53.9
13:35:47.98 +56:25:26.9
13:29:39.32 +57:46:53.7
13:37:33.57 +57:53:54.2
13:19:43.59 +57:38:24.6
13:27:52.42 +56:39:14.1
13:30:35.53 +56:25:59.8
13:29:49.51 +55:55:24.1
13:27:33.19 +57:11:01.1
13:24:55.69 +58:02:03.5
13:25:06.01 +56:03:55.8
13:30:45.23 +56:10:21.4
13:32:33.97 +58:04:59.5
13:24:10.58 +55:55:38.0
13:19:12.46 +57:54:48.1
13:34:38.50 +55:02:23.1
13:35:00.05 +54:19:57.5
13:33:49.07 +57:11:48.0
13:30:06.85 +55:32:44.9
13:33:07.59 +56:55:09.2
13:34:02.26 +53:45:49.8
13:26:11.95 +58:08:48.1
13:34:12.82 +57:23:34.5
13:21:34.24 +57:24:00.9
13:33:16.68 +56:02:20.7
13:22:34.87 +57:07:00.1
13:16:58.90 +57:58:46.2
13:32:12.73 +56:43:21.7
13:26:27.45 +55:31:27.0
13:37:20.82 +57:42:57.3
13:20:40.79 +56:16:55.4
13:32:35.65 +56:43:00.5
13:32:39.41 +56:21:47.7
13:29:32.26 +56:38:56.3
13:27:36.74 +56:54:51.3
13:16:26.33 +58:23:20.5
13:24:35.97 +55:42:48.2
13:29:31.07 +54:28:48.1
13:35:42.07 +55:39:46.8
13:31:38.23 +57:46:45.5
13:35:17.16 +57:09:30.3
13:25:32.35 +57:02:27.0
13:28:57.34 +54:55:28.8
13:20:38.43 +58:20:20.3
13:17:31.54 +57:40:15.0
13:32:12.43 +55:41:13.6
13:15:06.49 +58:19:32.4
13:30:04.64 +54:05:47.9
13:35:36.63 +56:26:44.6
13:31:59.09 +53:43:16.7
13:26:52.16 +56:17:06.8
13:31:49.34 +54:25:39.5
13:26:07.48 +57:07:15.2
13:29:41.46 +54:26:58.1
13:35:29.99 +55:58:19.5
13:35:36.17 +57:42:23.5
13:23:06.20 +56:58:04.7
13:33:05.99 +56:01:54.6
13:30:08.92 +55:07:45.3
13:35:28.25 +55:30:37.3
13:29:42.05 +57:05:43.8
13:26:36.20 +57:53:55.1
13:35:11.81 +54:56:50.8
13:26:09.81 +58:11:20.2
13:37:43.90 +57:49:36.4
13:35:02.96 +55:22:48.2
13:32:30.14 +55:07:47.4
13:34:18.21 +56:21:11.8
13:34:48.59 +57:26:06.3
13:27:17.06 +56:28:03.0
13:30:51.98 +57:50:11.6
13:28:37.91 +56:47:39.1
13:25:34.74 +57:55:45.3
13:28:25.05 +55:52:20.8
13:27:59.57 +56:11:43.2
13:36:11.79 +55:41:07.1
13:36:03.90 +55:45:03.5
13:28:32.27 +57:16:13.5
13:29:31.13 +54:38:43.4
13:25:31.18 +57:34:57.9
13:27:09.74 +55:21:59.7
13:19:57.09 +57:14:25.4
13:27:58.43 +56:06:08.1
13:33:15.68 +55:22:25.9
13:34:38.85 +57:20:06.3
13:17:19.63 +57:39:02.2
13:27:32.49 +54:55:50.9
13:13:07.06 +58:17:02.6
13:33:02.67 +58:01:04.6
13:32:21.75 +56:49:55.0
13:28:12.62 +55:29:03.5
13:33:14.41 +56:51:02.5
13:30:10.43 +55:54:10.4
13:29:09.05 +57:22:17.2
13:27:38.84 +54:49:37.0
13:28:49.36 +57:05:53.9
13:26:36.05 +55:46:30.0
13:26:09.73 +55:23:20.2
###################################################################################
13:34:41.89 +54:41:13.1 -- not an asteroid (will add it to exclusion list)
13:25:55.53 +54:55:18.2 -- not an asteroid (will add it to exclusion list)
13:30:14.92 +56:36:07.6 -- not an asteroid (will add it to exclusion list)
13:31:15.03 +57:33:48.2 -- not an asteroid (will add it to exclusion list)
13:26:02.28 +57:11:14.2 -- not an asteroid (will add it to exclusion list)
13:15:30.00 +58:34:02.4 -- not an asteroid (will add it to exclusion list)
13:33:48.65 +56:21:08.6 -- not an asteroid (will add it to exclusion list)
13:19:45.22 +57:36:44.1 -- not an asteroid (will add it to exclusion list)
13:27:59.91 +56:39:40.6 -- not an asteroid (will add it to exclusion list)
13:30:16.46 +55:57:24.3 -- not an asteroid (will add it to exclusion list)
13:24:40.14 +55:43:16.2 -- not an asteroid (will add it to exclusion list)
13:25:48.19 +57:15:25.8 -- not an asteroid (will add it to exclusion list)
13:34:20.56 +54:34:42.8 -- not an asteroid (will add it to exclusion list)
13:34:29.99 +54:15:13.6 -- not an asteroid (will add it to exclusion list)
13:23:16.05 +56:22:41.7 -- not an asteroid (will add it to exclusion list)
13:34:27.04 +53:08:32.6 -- not an asteroid (will add it to exclusion list)
13:29:45.28 +54:22:32.6 -- not an asteroid (will add it to exclusion list)
13:28:11.42 +57:27:17.9 -- not an asteroid (will add it to exclusion list)
13:17:30.73 +57:37:26.8 -- not an asteroid (will add it to exclusion list)
13:31:31.66 +57:20:57.0 -- not an asteroid (will add it to exclusion list)
13:36:04.83 +55:33:13.9 -- not an asteroid (will add it to exclusion list)
13:30:19.90 +56:33:19.9 -- not an asteroid (will add it to exclusion list)
13:31:13.88 +56:14:46.3 -- not an asteroid (will add it to exclusion list)
13:25:43.05 +57:29:37.5 -- not an asteroid (will add it to exclusion list)
13:36:16.05 +56:34:35.0 -- not an asteroid (will add it to exclusion list)
13:29:48.87 +57:29:40.5 -- not an asteroid (will add it to exclusion list)
13:33:46.98 +55:05:27.0 -- not an asteroid (will add it to exclusion list)
13:22:49.06 +57:08:53.9 -- not an asteroid (will add it to exclusion list)
13:35:47.98 +56:25:26.9 -- not an asteroid (will add it to exclusion list)
13:29:39.32 +57:46:53.7 -- not an asteroid (will add it to exclusion list)
13:37:33.57 +57:53:54.2 -- not an asteroid (will add it to exclusion list)
13:19:43.59 +57:38:24.6 -- not an asteroid (will add it to exclusion list)
13:27:52.42 +56:39:14.1 -- not an asteroid (will add it to exclusion list)
13:30:35.53 +56:25:59.8 -- not an asteroid (will add it to exclusion list)
13:29:49.51 +55:55:24.1 -- not an asteroid (will add it to exclusion list)
13:27:33.19 +57:11:01.1 -- not an asteroid (will add it to exclusion list)
13:24:55.69 +58:02:03.5 -- not an asteroid (will add it to exclusion list)
13:25:06.01 +56:03:55.8 -- not an asteroid (will add it to exclusion list)
13:30:45.23 +56:10:21.4 -- not an asteroid (will add it to exclusion list)
13:32:33.97 +58:04:59.5 -- not an asteroid (will add it to exclusion list)
13:24:10.58 +55:55:38.0 -- not an asteroid (will add it to exclusion list)
13:19:12.46 +57:54:48.1 -- not an asteroid (will add it to exclusion list)
13:34:38.50 +55:02:23.1 -- not an asteroid (will add it to exclusion list)
13:35:00.05 +54:19:57.5 -- not an asteroid (will add it to exclusion list)
13:33:49.07 +57:11:48.0 -- not an asteroid (will add it to exclusion list)
13:30:06.85 +55:32:44.9 -- not an asteroid (will add it to exclusion list)
13:33:07.59 +56:55:09.2 -- not an asteroid (will add it to exclusion list)
13:34:02.26 +53:45:49.8 -- not an asteroid (will add it to exclusion list)
13:26:11.95 +58:08:48.1 -- not an asteroid (will add it to exclusion list)
13:34:12.82 +57:23:34.5 -- not an asteroid (will add it to exclusion list)
13:21:34.24 +57:24:00.9 -- not an asteroid (will add it to exclusion list)
13:33:16.68 +56:02:20.7 -- not an asteroid (will add it to exclusion list)
13:22:34.87 +57:07:00.1 -- not an asteroid (will add it to exclusion list)
13:16:58.90 +57:58:46.2 -- not an asteroid (will add it to exclusion list)
13:32:12.73 +56:43:21.7 -- not an asteroid (will add it to exclusion list)
13:26:27.45 +55:31:27.0 -- not an asteroid (will add it to exclusion list)
13:37:20.82 +57:42:57.3 -- not an asteroid (will add it to exclusion list)
13:20:40.79 +56:16:55.4 -- not an asteroid (will add it to exclusion list)
13:32:35.65 +56:43:00.5 -- not an asteroid (will add it to exclusion list)
13:32:39.41 +56:21:47.7 -- not an asteroid (will add it to exclusion list)
13:29:32.26 +56:38:56.3 -- not an asteroid (will add it to exclusion list)
13:27:36.74 +56:54:51.3 -- not an asteroid (will add it to exclusion list)
13:16:26.33 +58:23:20.5 -- not an asteroid (will add it to exclusion list)
13:24:35.97 +55:42:48.2 -- not an asteroid (will add it to exclusion list)
13:29:31.07 +54:28:48.1 -- not an asteroid (will add it to exclusion list)
13:35:42.07 +55:39:46.8 -- not an asteroid (will add it to exclusion list)
13:31:38.23 +57:46:45.5 -- not an asteroid (will add it to exclusion list)
13:35:17.16 +57:09:30.3 -- not an asteroid (will add it to exclusion list)
13:25:32.35 +57:02:27.0 -- not an asteroid (will add it to exclusion list)
13:28:57.34 +54:55:28.8 -- not an asteroid (will add it to exclusion list)
13:20:38.43 +58:20:20.3 -- not an asteroid (will add it to exclusion list)
13:17:31.54 +57:40:15.0 -- not an asteroid (will add it to exclusion list)
13:32:12.43 +55:41:13.6 -- not an asteroid (will add it to exclusion list)
13:15:06.49 +58:19:32.4 -- not an asteroid (will add it to exclusion list)
13:30:04.64 +54:05:47.9 -- not an asteroid (will add it to exclusion list)
13:35:36.63 +56:26:44.6 -- not an asteroid (will add it to exclusion list)
13:31:59.09 +53:43:16.7 -- not an asteroid (will add it to exclusion list)
13:26:52.16 +56:17:06.8 -- not an asteroid (will add it to exclusion list)
13:31:49.34 +54:25:39.5 -- not an asteroid (will add it to exclusion list)
13:26:07.48 +57:07:15.2 -- not an asteroid (will add it to exclusion list)
13:29:41.46 +54:26:58.1 -- not an asteroid (will add it to exclusion list)
13:35:29.99 +55:58:19.5 -- not an asteroid (will add it to exclusion list)
13:35:36.17 +57:42:23.5 -- not an asteroid (will add it to exclusion list)
13:23:06.20 +56:58:04.7 -- not an asteroid (will add it to exclusion list)
13:33:05.99 +56:01:54.6 -- not an asteroid (will add it to exclusion list)
13:30:08.92 +55:07:45.3 -- not an asteroid (will add it to exclusion list)
13:35:28.25 +55:30:37.3 -- not an asteroid (will add it to exclusion list)
13:29:42.05 +57:05:43.8 -- not an asteroid (will add it to exclusion list)
13:26:36.20 +57:53:55.1 -- not an asteroid (will add it to exclusion list)
13:35:11.81 +54:56:50.8 -- not an asteroid (will add it to exclusion list)
13:26:09.81 +58:11:20.2 -- not an asteroid (will add it to exclusion list)
13:37:43.90 +57:49:36.4 -- not an asteroid (will add it to exclusion list)
13:35:02.96 +55:22:48.2 -- not an asteroid (will add it to exclusion list)
13:32:30.14 +55:07:47.4 -- not an asteroid (will add it to exclusion list)
13:34:18.21 +56:21:11.8 -- not an asteroid (will add it to exclusion list)
13:34:48.59 +57:26:06.3 -- not an asteroid (will add it to exclusion list)
13:27:17.06 +56:28:03.0 -- not an asteroid (will add it to exclusion list)
13:30:51.98 +57:50:11.6 -- not an asteroid (will add it to exclusion list)
13:28:37.91 +56:47:39.1 -- not an asteroid (will add it to exclusion list)
13:25:34.74 +57:55:45.3 -- not an asteroid (will add it to exclusion list)
13:28:25.05 +55:52:20.8 -- not an asteroid (will add it to exclusion list)
13:27:59.57 +56:11:43.2 -- not an asteroid (will add it to exclusion list)
13:36:11.79 +55:41:07.1 -- not an asteroid (will add it to exclusion list)
13:36:03.90 +55:45:03.5 -- not an asteroid (will add it to exclusion list)
13:28:32.27 +57:16:13.5 -- not an asteroid (will add it to exclusion list)
13:29:31.13 +54:38:43.4 -- not an asteroid (will add it to exclusion list)
13:25:31.18 +57:34:57.9 -- not an asteroid (will add it to exclusion list)
13:27:09.74 +55:21:59.7 -- not an asteroid (will add it to exclusion list)
13:19:57.09 +57:14:25.4 -- not an asteroid (will add it to exclusion list)
13:27:58.43 +56:06:08.1 -- not an asteroid (will add it to exclusion list)
13:33:15.68 +55:22:25.9 -- not an asteroid (will add it to exclusion list)
13:34:38.85 +57:20:06.3 -- not an asteroid (will add it to exclusion list)
13:17:19.63 +57:39:02.2 -- not an asteroid (will add it to exclusion list)
13:27:32.49 +54:55:50.9 -- not an asteroid (will add it to exclusion list)
13:13:07.06 +58:17:02.6 -- not an asteroid (will add it to exclusion list)
13:33:02.67 +58:01:04.6 -- not an asteroid (will add it to exclusion list)
13:32:21.75 +56:49:55.0 -- not an asteroid (will add it to exclusion list)
13:28:12.62 +55:29:03.5 -- not an asteroid (will add it to exclusion list)
13:33:14.41 +56:51:02.5 -- not an asteroid (will add it to exclusion list)
13:30:10.43 +55:54:10.4 -- not an asteroid (will add it to exclusion list)
13:29:09.05 +57:22:17.2 -- not an asteroid (will add it to exclusion list)
13:27:38.84 +54:49:37.0 -- not an asteroid (will add it to exclusion list)
13:28:49.36 +57:05:53.9 -- not an asteroid (will add it to exclusion list)
13:26:36.05 +55:46:30.0 -- not an asteroid (will add it to exclusion list)
13:26:09.73 +55:23:20.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
13:13:07.06 +58:17:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:06.49 +58:19:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:30.00 +58:34:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:26.33 +58:23:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:58.90 +57:58:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:19.63 +57:39:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:30.73 +57:37:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:31.54 +57:40:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:12.46 +57:54:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:43.59 +57:38:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:45.22 +57:36:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:57.09 +57:14:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:38.43 +58:20:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:40.79 +56:16:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:34.24 +57:24:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:34.87 +57:07:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:49.06 +57:08:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:06.20 +56:58:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:16.05 +56:22:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:10.58 +55:55:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:35.97 +55:42:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:40.14 +55:43:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:55.69 +58:02:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:06.01 +56:03:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:31.18 +57:34:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:32.35 +57:02:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:34.74 +57:55:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:43.05 +57:29:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:48.19 +57:15:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:55.53 +54:55:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:02.28 +57:11:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:07.48 +57:07:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:09.73 +55:23:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:09.81 +58:11:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:11.95 +58:08:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:27.45 +55:31:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:36.05 +55:46:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:36.20 +57:53:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:52.16 +56:17:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:09.74 +55:21:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:17.06 +56:28:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:32.49 +54:55:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:33.19 +57:11:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:36.74 +56:54:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:38.84 +54:49:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:52.42 +56:39:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:58.43 +56:06:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:59.57 +56:11:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:59.91 +56:39:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:11.42 +57:27:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:12.62 +55:29:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:25.05 +55:52:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:32.27 +57:16:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:37.91 +56:47:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:49.36 +57:05:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:57.34 +54:55:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:09.05 +57:22:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:31.07 +54:28:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:31.13 +54:38:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:32.26 +56:38:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:39.32 +57:46:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:41.46 +54:26:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:42.05 +57:05:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:45.28 +54:22:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:48.87 +57:29:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:49.51 +55:55:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:04.64 +54:05:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:06.85 +55:32:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:08.92 +55:07:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:10.43 +55:54:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:14.92 +56:36:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:16.46 +55:57:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:19.90 +56:33:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:35.53 +56:25:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:45.23 +56:10:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:51.98 +57:50:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:13.88 +56:14:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:15.03 +57:33:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:31.66 +57:20:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:38.23 +57:46:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:49.34 +54:25:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:59.09 +53:43:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:12.43 +55:41:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:12.73 +56:43:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:21.75 +56:49:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:30.14 +55:07:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:33.97 +58:04:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:35.65 +56:43:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:39.41 +56:21:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:02.67 +58:01:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:05.99 +56:01:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:07.59 +56:55:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:14.41 +56:51:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:15.68 +55:22:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:16.68 +56:02:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:46.98 +55:05:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:48.65 +56:21:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:49.07 +57:11:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:02.26 +53:45:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:12.82 +57:23:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:18.21 +56:21:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:20.56 +54:34:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:27.04 +53:08:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:29.99 +54:15:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:38.50 +55:02:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:38.85 +57:20:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:41.89 +54:41:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:48.59 +57:26:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:00.05 +54:19:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:02.96 +55:22:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:11.81 +54:56:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:17.16 +57:09:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:28.25 +55:30:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:29.99 +55:58:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:36.17 +57:42:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:36.63 +56:26:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:42.07 +55:39:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:47.98 +56:25:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:03.90 +55:45:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:04.83 +55:33:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:11.79 +55:41:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:16.05 +56:34:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:37:20.82 +57:42:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:37:33.57 +57:53:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:37:43.90 +57:49:36.4 -- 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)
13:13:07.06 +58:17:02.6 -- not a known variable star
13:15:06.49 +58:19:32.4 -- not a known variable star
13:15:30.00 +58:34:02.4 -- not a known variable star
13:16:26.33 +58:23:20.5 -- not a known variable star
13:16:58.90 +57:58:46.2 -- not a known variable star
13:17:19.63 +57:39:02.2 -- not a known variable star
13:17:30.73 +57:37:26.8 -- not a known variable star
13:17:31.54 +57:40:15.0 -- not a known variable star
13:19:12.46 +57:54:48.1 -- not a known variable star
13:19:43.59 +57:38:24.6 -- not a known variable star
13:19:45.22 +57:36:44.1 -- not a known variable star
13:19:57.09 +57:14:25.4 -- not a known variable star
13:20:38.43 +58:20:20.3 -- not a known variable star
13:20:40.79 +56:16:55.4 -- not a known variable star
13:21:34.24 +57:24:00.9 -- not a known variable star
13:22:34.87 +57:07:00.1 -- not a known variable star
13:22:49.06 +57:08:53.9 -- a known variable star
13:23:06.20 +56:58:04.7 -- not a known variable star
13:23:16.05 +56:22:41.7 -- not a known variable star
13:24:10.58 +55:55:38.0 -- not a known variable star
13:24:35.97 +55:42:48.2 -- a known variable star
13:24:40.14 +55:43:16.2 -- not a known variable star
13:24:55.69 +58:02:03.5 -- not a known variable star
13:25:06.01 +56:03:55.8 -- not a known variable star
13:25:31.18 +57:34:57.9 -- not a known variable star
13:25:32.35 +57:02:27.0 -- not a known variable star
13:25:34.74 +57:55:45.3 -- not a known variable star
13:25:43.05 +57:29:37.5 -- not a known variable star
13:25:48.19 +57:15:25.8 -- not a known variable star
13:25:55.53 +54:55:18.2 -- not a known variable star
13:26:02.28 +57:11:14.2 -- not a known variable star
13:26:07.48 +57:07:15.2 -- not a known variable star
13:26:09.73 +55:23:20.2 -- not a known variable star
13:26:09.81 +58:11:20.2 -- not a known variable star
13:26:11.95 +58:08:48.1 -- not a known variable star
13:26:27.45 +55:31:27.0 -- not a known variable star
13:26:36.05 +55:46:30.0 -- not a known variable star
13:26:36.20 +57:53:55.1 -- not a known variable star
13:26:52.16 +56:17:06.8 -- not a known variable star
13:27:09.74 +55:21:59.7 -- not a known variable star
13:27:17.06 +56:28:03.0 -- not a known variable star
13:27:32.49 +54:55:50.9 -- not a known variable star
13:27:33.19 +57:11:01.1 -- not a known variable star
13:27:36.74 +56:54:51.3 -- not a known variable star
13:27:38.84 +54:49:37.0 -- not a known variable star
13:27:52.42 +56:39:14.1 -- not a known variable star
13:27:58.43 +56:06:08.1 -- not a known variable star
13:27:59.57 +56:11:43.2 -- not a known variable star
13:27:59.91 +56:39:40.6 -- not a known variable star
13:28:11.42 +57:27:17.9 -- not a known variable star
13:28:12.62 +55:29:03.5 -- not a known variable star
13:28:25.05 +55:52:20.8 -- not a known variable star
13:28:32.27 +57:16:13.5 -- not a known variable star
13:28:37.91 +56:47:39.1 -- not a known variable star
13:28:49.36 +57:05:53.9 -- not a known variable star
13:28:57.34 +54:55:28.8 -- not a known variable star
13:29:09.05 +57:22:17.2 -- not a known variable star
13:29:31.07 +54:28:48.1 -- not a known variable star
13:29:31.13 +54:38:43.4 -- not a known variable star
13:29:32.26 +56:38:56.3 -- not a known variable star
13:29:39.32 +57:46:53.7 -- not a known variable star
13:29:41.46 +54:26:58.1 -- not a known variable star
13:29:42.05 +57:05:43.8 -- not a known variable star
13:29:45.28 +54:22:32.6 -- not a known variable star
13:29:48.87 +57:29:40.5 -- not a known variable star
13:29:49.51 +55:55:24.1 -- not a known variable star
13:30:04.64 +54:05:47.9 -- not a known variable star
13:30:06.85 +55:32:44.9 -- not a known variable star
13:30:08.92 +55:07:45.3 -- not a known variable star
13:30:10.43 +55:54:10.4 -- not a known variable star
13:30:14.92 +56:36:07.6 -- not a known variable star
13:30:16.46 +55:57:24.3 -- a known variable star
13:30:19.90 +56:33:19.9 -- not a known variable star
13:30:35.53 +56:25:59.8 -- not a known variable star
13:30:45.23 +56:10:21.4 -- not a known variable star
13:30:51.98 +57:50:11.6 -- not a known variable star
13:31:13.88 +56:14:46.3 -- not a known variable star
13:31:15.03 +57:33:48.2 -- not a known variable star
13:31:31.66 +57:20:57.0 -- a known variable star
13:31:38.23 +57:46:45.5 -- not a known variable star
13:31:49.34 +54:25:39.5 -- not a known variable star
13:31:59.09 +53:43:16.7 -- not a known variable star
13:32:12.43 +55:41:13.6 -- not a known variable star
13:32:12.73 +56:43:21.7 -- not a known variable star
13:32:21.75 +56:49:55.0 -- not a known variable star
13:32:30.14 +55:07:47.4 -- not a known variable star
13:32:33.97 +58:04:59.5 -- not a known variable star
13:32:35.65 +56:43:00.5 -- not a known variable star
13:32:39.41 +56:21:47.7 -- not a known variable star
13:33:02.67 +58:01:04.6 -- not a known variable star
13:33:05.99 +56:01:54.6 -- not a known variable star
13:33:07.59 +56:55:09.2 -- not a known variable star
13:33:14.41 +56:51:02.5 -- not a known variable star
13:33:15.68 +55:22:25.9 -- not a known variable star
13:33:16.68 +56:02:20.7 -- not a known variable star
13:33:46.98 +55:05:27.0 -- not a known variable star
13:33:48.65 +56:21:08.6 -- not a known variable star
13:33:49.07 +57:11:48.0 -- not a known variable star
13:34:02.26 +53:45:49.8 -- not a known variable star
13:34:12.82 +57:23:34.5 -- not a known variable star
13:34:18.21 +56:21:11.8 -- not a known variable star
13:34:20.56 +54:34:42.8 -- not a known variable star
13:34:27.04 +53:08:32.6 -- not a known variable star
13:34:29.99 +54:15:13.6 -- not a known variable star
13:34:38.50 +55:02:23.1 -- not a known variable star
13:34:38.85 +57:20:06.3 -- not a known variable star
13:34:41.89 +54:41:13.1 -- not a known variable star
13:34:48.59 +57:26:06.3 -- not a known variable star
13:35:00.05 +54:19:57.5 -- not a known variable star
13:35:02.96 +55:22:48.2 -- not a known variable star
13:35:11.81 +54:56:50.8 -- not a known variable star
13:35:17.16 +57:09:30.3 -- not a known variable star
13:35:28.25 +55:30:37.3 -- not a known variable star
13:35:29.99 +55:58:19.5 -- not a known variable star
13:35:36.17 +57:42:23.5 -- not a known variable star
13:35:36.63 +56:26:44.6 -- not a known variable star
13:35:42.07 +55:39:46.8 -- not a known variable star
13:35:47.98 +56:25:26.9 -- not a known variable star
13:36:03.90 +55:45:03.5 -- not a known variable star
13:36:04.83 +55:33:13.9 -- not a known variable star
13:36:11.79 +55:41:07.1 -- not a known variable star
13:36:16.05 +56:34:35.0 -- not a known variable star
13:37:20.82 +57:42:57.3 -- not a known variable star
13:37:33.57 +57:53:54.2 -- not a known variable star
13:37:43.90 +57:49:36.4 -- not a known variable star
Found 121 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
125 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 125 (excluding asteroids and hot pixels, 121 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461258.69845010 -observatory V36
07:45:30.66 +20:23:14.0 Mercury (-0.3mag)
11:55:36.57 -00:03:23.2 Venus (-4.3mag)
05:43:22.67 +23:32:37.0 Mars (1.3mag)
08:41:06.98 +18:48:02.4 Jupiter (-1.8mag)
00:56:33.04 +03:16:47.9 Saturn (0.6mag)
04:11:29.55 +20:56:20.2 Uranus (5.8mag)
00:16:12.86 +00:13:59.3 Neptune (7.7mag)
20:28:20.12 -23:29:23.7 Pluto (14.4mag)
02:45:34.75 +20:27:58.5 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Aug 5 23:50 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461258.69845010:
08:41:14.09 +18:47:32.2 Io (6.0mag)
08:41:04.04 +18:48:15.4 Europa (6.3mag)
08:41:03.23 +18:48:22.4 Ganymede (5.6mag)
08:40:53.05 +18:49:05.0 Callisto (6.7mag)
08:38:42.88 +18:46:11.5 Himalia (15.7mag)
08:41:05.41 +18:48:10.0 Thebe (16.6mag)
08:38:13.51 +18:45:07.1 Elara (17.7mag)
08:45:12.87 +18:28:27.7 Pasiphae (17.9mag)
08:44:25.87 +18:57:52.5 Carme (19.0mag)
00:56:30.91 +03:17:14.8 Titan (8.4mag)
00:56:27.36 +03:16:51.9 Rhea (9.7mag)
00:56:36.62 +03:15:09.8 Iapetus (11.1mag)
00:56:19.68 +03:17:02.4 Hyperion (14.4mag)
00:55:58.11 +03:10:14.8 Phoebe (16.5mag)
-rw-r--r-- 1 apache apache 568 Aug 5 23:51 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461258.69845010:
18:55:37.94 -24:04:11.8 JWST
17:12:47.10 +42:17:52.5 Chandra
09:16:21.72 -52:21:08.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 5 23:50 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461258.69845010 -observatory V36
03:11:21.73 +17:12:19.8 17.7mag P/1996 R2 (Lagerkvist)
18:02:25.02 -34:38:24.4 14.0mag P/2010 H2 (Vales)
06:51:53.72 -68:49:36.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:09:16.67 +32:57:03.5 17.7mag C/2017 K2 (PANSTARRS)
03:37:38.79 +36:43:13.0 16.7mag P/2021 N1 (ZTF)
22:40:17.86 +31:34:00.6 17.3mag C/2022 E2 (ATLAS)
06:41:27.48 +26:34:32.8 16.8mag C/2022 N2 (PANSTARRS)
10:19:41.68 +28:33:38.9 17.0mag C/2022 QE78 (ATLAS)
09:27:30.14 +05:17:43.1 17.9mag C/2022 R6 (PANSTARRS)
15:12:08.99 -12:12:25.4 17.9mag P/2023 B1 (PANSTARRS)
21:13:26.96 +66:14:03.4 17.9mag C/2023 H5 (Lemmon)
15:49:55.82 -12:44:48.6 14.3mag C/2023 R1 (PANSTARRS)
08:05:48.57 +31:15:16.9 15.2mag C/2024 E1 (Wierzchos)
15:07:18.03 +15:36:58.9 17.7mag C/2024 G6 (ATLAS)
19:05:42.24 +42:57:36.5 13.7mag C/2024 J3 (ATLAS)
21:13:42.19 +49:04:36.7 17.6mag C/2024 R4 (PANSTARRS)
05:13:30.18 -12:59:39.5 15.5mag C/2024 T5 (ATLAS)
06:54:53.93 +24:30:43.9 17.9mag C/2025 J1 (Borisov)
07:29:56.25 -15:51:49.3 17.7mag C/2025 R3 (PANSTARRS)
10:30:05.53 +21:01:57.6 17.3mag C/2025 V2 (Rankin)
12:56:55.57 +02:29:01.2 17.0mag C/2025 Y1 (ATLAS)
16:03:42.77 +78:01:14.8 16.8mag C/2026 A2 (Bok)
03:06:42.38 +46:08:40.7 17.1mag C/2026 B2 (Sun-Gao)
11:45:07.62 +08:19:47.4 17.3mag A/2026 E1
21:56:05.42 -26:26:43.7 6.9mag 10P/Tempel
11:27:45.13 -03:16:29.9 16.2mag 29P/Schwassmann-Wachmann
04:36:43.51 +32:15:34.9 18.0mag 47P/Ashbrook-Jackson
11:03:33.41 +05:18:17.5 17.2mag 63P/Wild
00:54:17.95 -05:22:39.6 15.4mag 65P/Gunn
05:30:56.59 +20:43:47.4 13.7mag 78P/Gehrels
20:39:48.94 -23:17:21.0 17.8mag 84P/Giclas
02:58:41.88 +13:32:15.5 16.7mag 88P/Howell
07:50:41.79 +27:55:54.4 16.1mag 93P/Lovas
04:00:39.67 +16:05:12.2 17.6mag 112P/Urata-Niijima
05:49:47.02 +30:31:01.3 16.3mag 114P/Wiseman-Skiff
09:13:41.18 +26:59:24.9 15.0mag 123P/West-Hartley
11:39:41.00 -09:29:18.9 17.1mag 124P/Mrkos
05:33:33.54 +21:11:10.6 16.1mag 128P/Shoemaker-Holt
06:25:02.39 +18:59:50.3 17.9mag 131P/Mueller
00:03:42.05 +03:25:22.1 17.6mag 139P/Vaisala-Oterma
03:21:34.42 -19:44:57.4 14.0mag 161P/Hartley-IRAS
07:09:08.96 +37:41:17.4 15.8mag 162P/SidingSpring
15:50:22.62 +39:28:20.0 12.3mag 169P/NEAT
02:39:15.48 +09:28:29.4 17.6mag 220P/McNaught
16:40:34.63 -09:56:33.6 17.6mag 235P/LINEAR
20:23:45.19 -52:50:55.2 17.8mag 259P/Garradd
03:16:12.58 +24:18:31.1 15.4mag 260P/McNaught
06:59:15.51 +37:45:18.4 17.3mag 295P/LINEAR
15:09:50.53 +03:21:42.1 17.7mag 391P/Kowalski
08:59:02.26 +18:28:31.0 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.5K Aug 5 23:50 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
-rw-r--r-- 1 apache apache 5.7K Aug 5 23:50 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
09:55:21.28 +69:02:52.6 PNV J09552128+6902526 2026-06-13.933 18.9mag
19:51:21.42 +37:06:40.0 TCP J19512142+3706400 2026-06-17.2942 16.8mag
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
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
-rw-r--r-- 1 apache apache 189K Aug 5 23:50 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
18:55:34.805 +34:42:05.78 AT 2026vky 2026-06-22.39 21.01
15:27:13.875 -10:50:21.14 AT 2026vkx 2026-06-14.35 20.55
13:36:43.476 +25:28:01.16 AT 2026vkw 2026-06-25.38 20.6
04:43:04.292 -16:08:54.64 AT 2026vkv 2026-01-12.30 21.72
04:48:25.928 -18:19:58.05 AT 2026vku 2026-01-26.25 21.35
12:55:24.686 +13:58:33.13 AT 2026vkt 2026-06-05.34 21.42
11:39:28.884 +47:23:59.43 AT 2026vks 2026-01-14.61 21.82
10:26:55.799 -14:09:20.42 AT 2026vkr 2026-01-13.55 21.98
12:26:22.284 +20:06:25.68 AT 2026vkq 2026-02-13.60 20.86
12:08:12.778 +41:30:56.83 AT 2026vkp 2026-06-15.27 20.88
05:11:50.298 -12:02:24.75 AT 2026vko 2026-02-15.23 20.49
00:35:37.087 -45:29:22.45 AT 2026vkn 2026-06-26.42 23.13
04:11:06.535 -49:23:35.67 AT 2026vkm 2026-07-09.42 22.31
23:40:19.411 -26:01:53.34 AT 2026vkl 2026-07-20.59 21.47
22:23:27.160 +00:54:32.97 AT 2026vkk 2026-07-14.55 21.17
21:14:05.875 -09:55:36.50 AT 2026vkj 2026-07-20.46 21.9
17:17:56.970 +19:09:32.22 AT 2026vki 2026-07-19.39 21.8
17:18:18.165 +24:21:20.44 AT 2026vkh 2026-07-19.40 21.78
18:14:11.533 +25:31:50.45 AT 2026vkg 2026-07-16.29 20.95
22:50:03.729 +40:38:42.44 AT 2026vkf 2026-07-20.53 20.32
-rw-r--r-- 1 apache apache 87K Aug 5 23:50 tns_transients_list.txt
