This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_UMa-03-Q1b1x1_055851_TTUQ1b1x1_2579400_WLmt4Jj0
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 22.4568 2461274.9568 11.95 10:09:56.10 +60:07:24.8
151.25687 47.14855 galactic UMa Second-epoch detections are separated by 1.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:56.10 +60:07:24.8 (user input) | T | P | (position from user input) J-Ks=0.567+/-0.030 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:09:56.10 +60:07:24.8: 12.85 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:09:56.10 +60:07:24.8: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 09 56.10 +60 07 24.8 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,11.95,0.05,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
target 20260822.4568 11.95CV 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 22.4568 2461274.9568 11.97 10:26:23.35 +61:07:26.3
148.32334 48.23106 galactic UMa Second-epoch detections are separated by 0.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:26:23.35 +61:07:26.3 (user input) | T | P | (position from user input) J-Ks=0.580+/-0.034 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:26:23.35 +61:07:26.3: 12.91 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:26:23.35 +61:07:26.3: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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 22.4568* 10 26 23.35 +61 07 26.3 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 11.97CV 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 22.4568 2461274.9568 12.02 10:29:50.96 +63:22:58.8
145.34762 47.11254 galactic UMa Second-epoch detections are separated by 0.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:29:50.96 +63:22:58.8 (user input) | T | P | (position from user input) J-Ks=0.258+/-0.034 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:29:50.96 +63:22:58.8: 12.93 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:29:50.96 +63:22:58.8: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 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 22.4568* 10 29 50.96 +63 22 58.8 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.02CV 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 22.4568 2461274.9568 12.09 10:14:35.88 +60:21:09.9
150.50999 47.51067 galactic UMa Second-epoch detections are separated by 1.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:14:35.88 +60:21:09.9 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.030 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:14:35.88 +60:21:09.9: 13.09 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:14:35.88 +60:21:09.9: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 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 22.4568* 10 14 35.88 +60 21 09.9 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.04 10:00:53.61 +58:41:07.5
153.92748 46.87385 galactic UMa Second-epoch detections are separated by 1.5" and 7.0 pix
The object was found in VSX 1" Gaia DR3 1046881308984908288
Type: ROT
# Max. Min./Amp. JD0 Period
12.810 G 12.860 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:00:53.61 +58:41:07.5: 13.12 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:00:53.61 +58:41:07.5: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 00 53.61 +58 41 07.5 12.0 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 1046881308984908288,2461274.9568,12.04,0.05,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 1046881308984908288 20260822.4568 12.04CV 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 22.4568 2461274.9568 12.20 10:18:28.95 +60:56:51.6
149.38449 47.56684 galactic UMa Second-epoch detections are separated by 1.8" and 6.9 pix
The object was found in VSX 6" Gaia DR3 1048628639120754176
Type: ROT
# Max. Min./Amp. JD0 Period
14.100 G 14.130 G M
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:18:28.95 +60:56:51.6: 13.12 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:18:28.95 +60:56:51.6: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 22.4568* 10 18 28.95 +60 56 51.6 12.2 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 1048628639120754176,2461274.9568,12.20,0.05,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 1048628639120754176 20260822.4568 12.20CV 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 22.4568 2461274.9568 12.11 10:12:57.86 +60:37:56.3
150.32968 47.18866 galactic UMa Second-epoch detections are separated by 1.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:57.86 +60:37:56.3 (user input) | T | P | (position from user input) J-Ks=0.397+/-0.034 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:12:57.86 +60:37:56.3: 13.14 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:12:57.86 +60:37:56.3: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 22.4568* 10 12 57.86 +60 37 56.3 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.11,0.05,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
target 20260822.4568 12.11CV 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 22.4568 2461274.9568 12.21 10:05:06.18 +59:27:47.4
152.54743 46.96833 galactic UMa Second-epoch detections are separated by 1.5" and 6.7 pix
The object was found in VSX 1" Gaia DR3 1046942400599647872
Type: ROT
# Max. Min./Amp. JD0 Period
12.900 G 12.950 G G
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:05:06.18 +59:27:47.4: 13.15 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:05:06.18 +59:27:47.4: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 05 06.18 +59 27 47.4 12.2 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 1046942400599647872,2461274.9568,12.21,0.05,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 1046942400599647872 20260822.4568 12.21CV 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 22.4568 2461274.9568 12.16 10:00:32.05 +59:26:27.5
152.99125 46.47342 galactic UMa Second-epoch detections are separated by 0.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:00:32.05 +59:26:27.5 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:00:32.05 +59:26:27.5: 13.16 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:00:32.05 +59:26:27.5: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 00 32.05 +59 26 27.5 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.16,0.05,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
target 20260822.4568 12.16CV 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 22.4568 2461274.9568 12.29 09:22:15.59 +64:30:48.0
149.41313 40.22801 galactic UMa Second-epoch detections are separated by 0.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:22:15.59 +64:30:48.0 (user input) | T | P | (position from user input) J-Ks=0.330+/-0.029 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:22:15.59 +64:30:48.0: 13.16 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:22:15.59 +64:30:48.0: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 22 15.59 +64 30 48.0 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.31 10:16:27.10 +62:14:32.0
148.04351 46.61775 galactic UMa Second-epoch detections are separated by 1.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:16:27.10 +62:14:32.0 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.032 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:16:27.10 +62:14:32.0: 13.21 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:16:27.10 +62:14:32.0: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 16 27.10 +62 14 32.0 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.31,0.05,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
target 20260822.4568 12.31CV 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 22.4568 2461274.9568 12.24 10:25:58.84 +62:11:55.0
147.10880 47.52842 galactic UMa Second-epoch detections are separated by 1.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:25:58.84 +62:11:55.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:25:58.84 +62:11:55.0: 13.23 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:25:58.84 +62:11:55.0: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 25 58.84 +62 11 55.0 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.28 10:08:56.14 +58:56:53.4
152.83727 47.65186 galactic UMa Second-epoch detections are separated by 5.1" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J152.2340+58.9480 | 10:08:56.14 +58:56:53.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.409+/-0.041 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:08:56.14 +58:56:53.4: 13.24 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:08:56.14 +58:56:53.4: 13.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 08 56.14 +58 56 53.4 12.3 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
ATO J152.2340+58.9480,2461274.9568,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J152.2340+58.9480 20260822.4568 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.35 10:02:06.48 +60:00:16.5
152.13719 46.37142 galactic UMa Second-epoch detections are separated by 2.8" and 7.1 pix
The object was found in VSX21" Gaia DR3 1050015569959219968
Type: ROT
# Max. Min./Amp. JD0 Period
14.240 G 14.280 G G
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:02:06.48 +60:00:16.5: 13.28 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:02:06.48 +60:00:16.5: 13.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 02 06.48 +60 00 16.5 12.3 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 1050015569959219968,2461274.9568,12.35,0.05,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 1050015569959219968 20260822.4568 12.35CV 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 22.4568 2461274.9568 12.32 10:16:18.66 +60:58:39.7
149.57143 47.33370 galactic UMa Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:16:18.66 +60:58:39.7 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.034 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:16:18.66 +60:58:39.7: 13.31 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:16:18.66 +60:58:39.7: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 16 18.66 +60 58 39.7 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.32,0.05,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
target 20260822.4568 12.32CV 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 22.4568 2461274.9568 12.41 09:15:44.90 +62:46:56.5
151.86821 40.18084 galactic UMa Second-epoch detections are separated by 1.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:15:44.90 +62:46:56.5 (user input) | T | P | (position from user input) J-Ks=0.302+/-0.030 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:15:44.90 +62:46:56.5: 13.33 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:15:44.90 +62:46:56.5: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 15 44.90 +62 46 56.5 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.45 10:25:29.57 +63:01:49.8
146.20670 46.96257 galactic UMa Second-epoch detections are separated by 2.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:25:29.57 +63:01:49.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:25:29.57 +63:01:49.8: 13.50 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:25:29.57 +63:01:49.8: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 25 29.57 +63 01 49.8 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.59 09:29:27.57 +65:31:50.6
147.78710 40.50679 galactic UMa Second-epoch detections are separated by 0.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx2099650 | 09:29:27.57 +65:31:50.6 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.569+/-0.028 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:29:27.57 +65:31:50.6: 13.58 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:29:27.57 +65:31:50.6: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 29 27.57 +65 31 50.6 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2099650,2461274.9568,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2099650 20260822.4568 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.51 09:14:01.47 +62:51:05.9
151.86878 39.97213 galactic UMa Second-epoch detections are separated by 2.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx2099947 | 09:14:01.47 +62:51:05.9 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:14:01.47 +62:51:05.9: 13.58 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:14:01.47 +62:51:05.9: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 14 01.47 +62 51 05.9 12.5 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
DocumentRef: VOTx2099947,2461274.9568,12.51,0.05,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
DocumentRef: VOTx2099947 20260822.4568 12.51CV 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 22.4568 2461274.9568 12.52 09:16:12.60 +62:25:51.4
152.27865 40.34884 galactic UMa Second-epoch detections are separated by 1.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:16:12.60 +62:25:51.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:16:12.60 +62:25:51.4: 13.58 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:16:12.60 +62:25:51.4: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 16 12.60 +62 25 51.4 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.52CV 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 22.4568 2461274.9568 12.43 10:17:14.42 +61:11:51.6
149.21051 47.29999 galactic UMa Second-epoch detections are separated by 2.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:17:14.42 +61:11:51.6 (user input) | T | P | (position from user input) J-Ks=0.465+/-0.032 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:17:14.42 +61:11:51.6: 13.58 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:17:14.42 +61:11:51.6: 13.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 17 14.42 +61 11 51.6 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.43,0.05,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
target 20260822.4568 12.43CV 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 22.4568 2461274.9568 12.62 09:12:36.44 +62:20:01.5
152.57712 39.98586 galactic UMa Second-epoch detections are separated by 1.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:12:36.44 +62:20:01.5 (user input) | T | P | (position from user input) J-Ks=0.813+/-0.030 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:12:36.44 +62:20:01.5: 13.77 +/- 0.05 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:12:36.44 +62:20:01.5: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 12 36.44 +62 20 01.5 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.66 09:18:53.59 +64:52:04.7
149.16457 39.76007 galactic UMa Second-epoch detections are separated by 0.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:18:53.59 +64:52:04.7 (user input) | T | P | (position from user input) J-Ks=0.286+/-0.033 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:18:53.59 +64:52:04.7: 13.74 +/- 0.05 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:18:53.59 +64:52:04.7: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 18 53.59 +64 52 04.7 12.7 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.45 10:01:47.99 +59:11:07.4
153.20403 46.73805 galactic UMa Second-epoch detections are separated by 1.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:01:47.99 +59:11:07.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.345+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:01:47.99 +59:11:07.4: 13.74 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:01:47.99 +59:11:07.4: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 01 47.99 +59 11 07.4 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.63 09:19:16.70 +64:13:48.8
149.91548 40.03677 galactic UMa Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:19:16.70 +64:13:48.8 (user input) | T | P | (position from user input) J-Ks=0.271+/-0.032 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:19:16.70 +64:13:48.8: 13.71 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:19:16.70 +64:13:48.8: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 19 16.70 +64 13 48.8 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.52 10:14:01.02 +60:38:09.5
150.22018 47.29421 galactic UMa Second-epoch detections are separated by 0.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:14:01.02 +60:38:09.5 (user input) | T | P | (position from user input) J-Ks=0.282+/-0.037 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:14:01.02 +60:38:09.5: 13.65 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:14:01.02 +60:38:09.5: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 14 01.02 +60 38 09.5 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.52CV 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 22.4568 2461274.9568 12.47 10:18:58.47 +61:47:58.7
148.31296 47.11725 galactic UMa Second-epoch detections are separated by 1.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:18:58.47 +61:47:58.7 (user input) | T | P | (position from user input) J-Ks=0.517+/-0.042 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:18:58.47 +61:47:58.7: 13.65 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:18:58.47 +61:47:58.7: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 18 58.47 +61 47 58.7 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.43 09:57:32.66 +58:51:43.9
153.99404 46.40740 galactic UMa Second-epoch detections are separated by 2.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:57:32.66 +58:51:43.9 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.441+/-0.035 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:57:32.66 +58:51:43.9: 13.63 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:57:32.66 +58:51:43.9: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 57 32.66 +58 51 43.9 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.43,0.05,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
target 20260822.4568 12.43CV 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 22.4568 2461274.9568 12.44 10:09:40.01 +61:21:23.2
149.76441 46.45753 galactic UMa Second-epoch detections are separated by 1.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:40.01 +61:21:23.2 (user input) | T | P | (position from user input) J-Ks=0.974+/-0.035 (M)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:09:40.01 +61:21:23.2: 13.59 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:09:40.01 +61:21:23.2: 13.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 09 40.01 +61 21 23.2 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.44,0.05,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
target 20260822.4568 12.44CV 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 22.4568 2461274.9568 12.58 09:35:34.28 +66:16:46.3
146.53749 40.73045 galactic UMa Second-epoch detections are separated by 1.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:35:34.28 +66:16:46.3 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.028 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:35:34.28 +66:16:46.3: 13.61 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:35:34.28 +66:16:46.3: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 35 34.28 +66 16 46.3 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.58,0.05,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
target 20260822.4568 12.58CV 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 22.4568 2461274.9568 12.39 10:04:12.93 +60:00:34.1
151.93980 46.59708 galactic UMa Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3045275 | 10:04:12.93 +60:00:34.1 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.510+/-0.031 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:04:12.93 +60:00:34.1: 13.56 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:04:12.93 +60:00:34.1: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 04 12.93 +60 00 34.1 12.4 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
DocumentRef: VOTx3045275,2461274.9568,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3045275 20260822.4568 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.53 09:10:23.61 +63:26:52.2
151.31092 39.38972 galactic UMa Second-epoch detections are separated by 2.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:10:23.61 +63:26:52.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:10:23.61 +63:26:52.2: 13.57 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:10:23.61 +63:26:52.2: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 10 23.61 +63 26 52.2 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.53,0.05,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
target 20260822.4568 12.53CV 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 22.4568 2461274.9568 12.44 10:09:43.41 +60:30:07.7
150.80716 46.92477 galactic UMa Second-epoch detections are separated by 3.3" and 7.1 pix
The object was found in VSX 7" Gaia DR3 1050105111438120576
Type: ROT
# Max. Min./Amp. JD0 Period
15.670 G 15.700 G K
ATTENTION: measured mag 12.44 is 3.2 mag brighter than the VSX record maximum brightness 15.67 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:09:43.41 +60:30:07.7: 13.57 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:09:43.41 +60:30:07.7: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 09 43.41 +60 30 07.7 12.4 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 1050105111438120576,2461274.9568,12.44,0.05,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 1050105111438120576 20260822.4568 12.44CV 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 22.4568 2461274.9568 12.50 09:21:44.85 +64:24:23.1
149.57020 40.21818 galactic UMa Second-epoch detections are separated by 3.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:21:44.85 +64:24:23.1 (user input) | T | P | (position from user input) J-Ks=0.607+/-0.029 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:21:44.85 +64:24:23.1: 13.56 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:21:44.85 +64:24:23.1: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 21 44.85 +64 24 23.1 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 22.4568 2461274.9568 12.46 10:30:00.03 +62:44:35.8
146.04871 47.54116 galactic UMa Second-epoch detections are separated by 2.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:30:00.03 +62:44:35.8 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.028 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:30:00.03 +62:44:35.8: 13.53 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:30:00.03 +62:44:35.8: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 30 00.03 +62 44 35.8 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.46,0.05,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
target 20260822.4568 12.46CV 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 22.4568 2461274.9568 12.57 09:21:57.62 +63:49:12.1
150.27030 40.46239 galactic UMa Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:21:57.62 +63:49:12.1 (user input) | T | P | (position from user input) J-Ks=0.581+/-0.071 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:21:57.62 +63:49:12.1: 13.55 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:21:57.62 +63:49:12.1: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 21 57.62 +63 49 12.1 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.57,0.05,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
target 20260822.4568 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.45 10:17:40.97 +61:31:06.9
148.77983 47.15763 galactic UMa Second-epoch detections are separated by 2.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3155921 | 10:17:40.97 +61:31:06.9 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.521+/-0.030 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:17:40.97 +61:31:06.9: 13.55 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:17:40.97 +61:31:06.9: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 17 40.97 +61 31 06.9 12.4 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
DocumentRef: VOTx3155921,2461274.9568,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3155921 20260822.4568 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.39 10:21:38.43 +61:02:07.5
148.94614 47.82614 galactic UMa Second-epoch detections are separated by 0.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J155.4103+61.0353 | 10:21:38.43 +61:02:07.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.427+/-0.052 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:21:38.43 +61:02:07.5: 13.51 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:21:38.43 +61:02:07.5: 13.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 21 38.43 +61 02 07.5 12.4 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
ATO J155.4103+61.0353,2461274.9568,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J155.4103+61.0353 20260822.4568 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.54 09:15:03.83 +64:59:59.6
149.20005 39.33445 galactic UMa Second-epoch detections are separated by 2.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:15:03.83 +64:59:59.6 (user input) | T | P | (position from user input) J-Ks=0.581+/-0.028 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:15:03.83 +64:59:59.6: 13.52 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:15:03.83 +64:59:59.6: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 15 03.83 +64 59 59.6 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.54,0.05,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
target 20260822.4568 12.54CV 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 22.4568 2461274.9568 12.42 09:17:12.51 +62:53:36.1
151.65709 40.29967 galactic UMa Second-epoch detections are separated by 1.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:17:12.51 +62:53:36.1 (user input) | T | P | (position from user input) J-Ks=0.685+/-0.028 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:17:12.51 +62:53:36.1: 13.50 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:17:12.51 +62:53:36.1: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 17 12.51 +62 53 36.1 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.42,0.05,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
target 20260822.4568 12.42CV 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 22.4568 2461274.9568 12.35 10:19:44.11 +61:26:10.0
148.66711 47.40457 galactic UMa Second-epoch detections are separated by 2.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3238393 | 10:19:44.11 +61:26:10.0 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.308+/-0.030 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:19:44.11 +61:26:10.0: 13.49 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:19:44.11 +61:26:10.0: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 19 44.11 +61 26 10.0 12.3 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
DocumentRef: VOTx3238393,2461274.9568,12.35,0.05,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
DocumentRef: VOTx3238393 20260822.4568 12.35CV 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 22.4568 2461274.9568 12.41 10:25:03.56 +61:25:13.7
148.11865 47.92325 galactic UMa Second-epoch detections are separated by 1.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:25:03.56 +61:25:13.7 (user input) | T | P | (position from user input) J-Ks=0.381+/-0.032 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:25:03.56 +61:25:13.7: 13.51 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:25:03.56 +61:25:13.7: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 25 03.56 +61 25 13.7 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.38 09:57:35.03 +59:35:02.8
153.06654 46.07616 galactic UMa Second-epoch detections are separated by 1.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:57:35.03 +59:35:02.8 (user input) | T | P | (position from user input) SpType: F8 (LAMOST DR5) J-Ks=0.324+/-0.037 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:57:35.03 +59:35:02.8: 13.48 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:57:35.03 +59:35:02.8: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 57 35.03 +59 35 02.8 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.38,0.05,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
target 20260822.4568 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.55 09:21:12.13 +63:39:58.8
150.49884 40.44210 galactic UMa Second-epoch detections are separated by 0.7" and 6.8 pix
The object was found in VSX 1" Gaia DR3 1067356311439043584
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.340 G 13.360 G F
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:21:12.13 +63:39:58.8: 13.48 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:21:12.13 +63:39:58.8: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 21 12.13 +63 39 58.8 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1067356311439043584,2461274.9568,12.55,0.05,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 1067356311439043584 20260822.4568 12.55CV 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 22.4568 2461274.9568 12.46 09:13:21.50 +63:36:01.9
150.98254 39.65115 galactic UMa Second-epoch detections are separated by 2.1" and 6.6 pix
The object was found in VSX 1" Gaia DR3 1043386202039153408
Type: ROT
# Max. Min./Amp. JD0 Period
13.300 G 13.310 G 0.498094000000 G
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:13:21.50 +63:36:01.9: 13.48 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:13:21.50 +63:36:01.9: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 13 21.50 +63 36 01.9 12.5 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 1043386202039153408,2461274.9568,12.46,0.05,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 1043386202039153408 20260822.4568 12.46CV 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 22.4568 2461274.9568 12.46 10:22:36.19 +62:25:55.7
147.19588 47.07571 galactic UMa Second-epoch detections are separated by 2.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3281975 | 10:22:36.19 +62:25:55.7 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.677+/-0.030 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:22:36.19 +62:25:55.7: 13.47 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:22:36.19 +62:25:55.7: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 22 36.19 +62 25 55.7 12.5 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
DocumentRef: VOTx3281975,2461274.9568,12.46,0.05,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
DocumentRef: VOTx3281975 20260822.4568 12.46CV 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 22.4568 2461274.9568 12.41 09:11:46.71 +62:38:39.3
152.23320 39.79629 galactic UMa Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1043201415365920896 | 09:11:46.71 +62:38:39.3 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.786+/-0.031 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:11:46.71 +62:38:39.3: 13.46 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:11:46.71 +62:38:39.3: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 11 46.71 +62 38 39.3 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1043201415365920896,2461274.9568,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1043201415365920896 20260822.4568 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.38 10:15:48.11 +61:20:12.1
149.18873 47.07864 galactic UMa Second-epoch detections are separated by 1.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:15:48.11 +61:20:12.1 (user input) | T | P | (position from user input) J-Ks=0.539+/-0.034 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:15:48.11 +61:20:12.1: 13.46 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:15:48.11 +61:20:12.1: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 15 48.11 +61 20 12.1 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.38,0.05,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
target 20260822.4568 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.54 09:12:25.54 +63:26:37.1
151.21967 39.60569 galactic UMa Second-epoch detections are separated by 1.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:12:25.54 +63:26:37.1 (user input) | T | P | (position from user input) SpType: M1 2011AJ....141...97W SDSS J091225.00+632643.7 J-Ks=0.274+/-0.036 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:12:25.54 +63:26:37.1: 13.45 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:12:25.54 +63:26:37.1: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 12 25.54 +63 26 37.1 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.54,0.05,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
target 20260822.4568 12.54CV 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 22.4568 2461274.9568 12.55 09:31:31.05 +65:17:30.6
147.94909 40.80309 galactic UMa Second-epoch detections are separated by 3.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:31:31.05 +65:17:30.6 (user input) | T | P | (position from user input) J-Ks=0.650+/-0.028 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:31:31.05 +65:17:30.6: 13.46 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:31:31.05 +65:17:30.6: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 31 31.05 +65 17 30.6 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.55,0.05,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
target 20260822.4568 12.55CV 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 22.4568 2461274.9568 12.32 10:18:02.98 +60:36:41.2
149.83801 47.71674 galactic UMa Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:18:02.98 +60:36:41.2 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.036 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:18:02.98 +60:36:41.2: 13.44 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:18:02.98 +60:36:41.2: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 18 02.98 +60 36 41.2 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.32,0.05,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
target 20260822.4568 12.32CV 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 22.4568 2461274.9568 12.37 10:07:54.95 +59:13:22.3
152.58613 47.39916 galactic UMa Second-epoch detections are separated by 1.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:07:54.95 +59:13:22.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.649+/-0.030 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:07:54.95 +59:13:22.3: 13.45 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:07:54.95 +59:13:22.3: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 07 54.95 +59 13 22.3 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.37,0.05,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
target 20260822.4568 12.37CV 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 22.4568 2461274.9568 12.33 10:31:02.44 +63:36:47.0
144.96460 47.06177 galactic UMa Second-epoch detections are separated by 1.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:31:02.44 +63:36:47.0 (user input) | T | P | (position from user input) J-Ks=0.611+/-0.028 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:31:02.44 +63:36:47.0: 13.45 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:31:02.44 +63:36:47.0: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 31 02.44 +63 36 47.0 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 22.4568 2461274.9568 12.45 09:09:19.97 +64:15:25.3
150.37299 39.01530 galactic UMa Second-epoch detections are separated by 2.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:09:19.97 +64:15:25.3 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.032 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:09:19.97 +64:15:25.3: 13.52 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:09:19.97 +64:15:25.3: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 09 19.97 +64 15 25.3 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.46 09:13:43.22 +62:51:10.3
151.88221 39.93898 galactic UMa Second-epoch detections are separated by 2.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3586687 | 09:13:43.22 +62:51:10.3 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.608+/-0.034 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:13:43.22 +62:51:10.3: 13.44 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:13:43.22 +62:51:10.3: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 13 43.22 +62 51 10.3 12.5 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
DocumentRef: VOTx3586687,2461274.9568,12.46,0.05,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
DocumentRef: VOTx3586687 20260822.4568 12.46CV 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 22.4568 2461274.9568 12.46 09:20:10.04 +63:43:52.2
150.47538 40.31162 galactic UMa Second-epoch detections are separated by 1.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3570451 | 09:20:10.04 +63:43:52.2 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.445+/-0.030 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:20:10.04 +63:43:52.2: 13.43 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:20:10.04 +63:43:52.2: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 20 10.04 +63 43 52.2 12.5 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
DocumentRef: VOTx3570451,2461274.9568,12.46,0.05,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
DocumentRef: VOTx3570451 20260822.4568 12.46CV 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 22.4568 2461274.9568 12.36 10:52:45.69 +64:57:24.9
141.09676 47.77046 galactic UMa Second-epoch detections are separated by 2.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:52:45.69 +64:57:24.9 (user input) | T | P | (position from user input) J-Ks=0.604+/-0.030 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:52:45.69 +64:57:24.9: 13.45 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:52:45.69 +64:57:24.9: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 52 45.69 +64 57 24.9 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.36,0.05,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
target 20260822.4568 12.36CV 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 22.4568 2461274.9568 12.44 10:15:54.42 +61:08:36.0
149.41166 47.19927 galactic UMa Second-epoch detections are separated by 3.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:15:54.42 +61:08:36.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:15:54.42 +61:08:36.0: 13.42 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:15:54.42 +61:08:36.0: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 15 54.42 +61 08 36.0 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.44,0.05,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
target 20260822.4568 12.44CV 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 22.4568 2461274.9568 12.42 09:13:51.94 +64:25:21.8
149.95670 39.42056 galactic UMa Second-epoch detections are separated by 1.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:13:51.94 +64:25:21.8 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.035 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:13:51.94 +64:25:21.8: 13.41 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:13:51.94 +64:25:21.8: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 13 51.94 +64 25 21.8 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.42,0.05,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
target 20260822.4568 12.42CV 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 22.4568 2461274.9568 12.42 09:21:24.76 +64:41:50.3
149.23694 40.07322 galactic UMa Second-epoch detections are separated by 1.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:21:24.76 +64:41:50.3 (user input) | T | P | (position from user input) J-Ks=0.577+/-0.024 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:21:24.76 +64:41:50.3: 13.41 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:21:24.76 +64:41:50.3: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 21 24.76 +64 41 50.3 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.42,0.05,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
target 20260822.4568 12.42CV 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 22.4568 2461274.9568 12.38 09:52:00.81 +58:34:14.1
154.83290 45.89472 galactic UMa Second-epoch detections are separated by 3.9" and 7.2 pix
The object was found in VSX 0" Gaia DR3 1049459698111859584
Type: ROT
# Max. Min./Amp. JD0 Period
13.110 G 13.130 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:52:00.81 +58:34:14.1: 13.40 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:52:00.81 +58:34:14.1: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 52 00.81 +58 34 14.1 12.4 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 1049459698111859584,2461274.9568,12.38,0.05,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 1049459698111859584 20260822.4568 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.34 10:07:46.74 +59:54:28.0
151.73420 47.03234 galactic UMa Second-epoch detections are separated by 0.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:07:46.74 +59:54:28.0 (user input) | T | P | (position from user input) J-Ks=0.640+/-0.033 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:07:46.74 +59:54:28.0: 13.41 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:07:46.74 +59:54:28.0: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 07 46.74 +59 54 28.0 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.45 09:15:49.88 +62:36:39.5
152.07540 40.24741 galactic UMa Second-epoch detections are separated by 0.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:15:49.88 +62:36:39.5 (user input) | T | P | (position from user input) J-Ks=0.325+/-0.030 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:15:49.88 +62:36:39.5: 13.40 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:15:49.88 +62:36:39.5: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 15 49.88 +62 36 39.5 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.38 10:34:54.53 +63:04:05.2
145.13979 47.74818 galactic UMa Second-epoch detections are separated by 1.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:34:54.53 +63:04:05.2 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:34:54.53 +63:04:05.2: 13.42 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:34:54.53 +63:04:05.2: 13.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 34 54.53 +63 04 05.2 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.38,0.05,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
target 20260822.4568 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.40 10:11:59.03 +60:47:46.8
150.22503 46.99838 galactic UMa Second-epoch detections are separated by 1.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:59.03 +60:47:46.8 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.032 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:11:59.03 +60:47:46.8: 13.40 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:11:59.03 +60:47:46.8: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 11 59.03 +60 47 46.8 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.40,0.05,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
target 20260822.4568 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.29 10:12:56.61 +58:55:04.6
152.47621 48.10970 galactic UMa Second-epoch detections are separated by 2.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:56.61 +58:55:04.6 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.028 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:12:56.61 +58:55:04.6: 13.39 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:12:56.61 +58:55:04.6: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 12 56.61 +58 55 04.6 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.40 10:10:28.32 +60:22:32.5
150.89128 47.07044 galactic UMa Second-epoch detections are separated by 1.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:28.32 +60:22:32.5 (user input) | T | P | (position from user input) J-Ks=0.425+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:10:28.32 +60:22:32.5: 13.38 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:10:28.32 +60:22:32.5: 13.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 10 28.32 +60 22 32.5 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.40,0.05,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
target 20260822.4568 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.23 10:25:26.20 +62:38:46.4
146.65126 47.19936 galactic UMa Second-epoch detections are separated by 1.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:25:26.20 +62:38:46.4 (user input) | T | P | (position from user input) J-Ks=0.399+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:25:26.20 +62:38:46.4: 13.37 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:25:26.20 +62:38:46.4: 13.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 25 26.20 +62 38 46.4 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.23,0.05,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
target 20260822.4568 12.23CV 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 22.4568 2461274.9568 12.34 10:10:17.45 +61:10:40.8
149.92229 46.61776 galactic UMa Second-epoch detections are separated by 0.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:17.45 +61:10:40.8 (user input) | T | P | (position from user input) J-Ks=0.689+/-0.031 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:10:17.45 +61:10:40.8: 13.34 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:10:17.45 +61:10:40.8: 13.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 10 17.45 +61 10 40.8 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.37 09:58:56.54 +58:40:26.8
154.11505 46.65495 galactic UMa Second-epoch detections are separated by 1.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx750412 | 09:58:56.54 +58:40:26.8 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:58:56.54 +58:40:26.8: 13.37 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:58:56.54 +58:40:26.8: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 58 56.54 +58 40 26.8 12.4 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
DocumentRef: VOTx750412,2461274.9568,12.37,0.05,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
DocumentRef: VOTx750412 20260822.4568 12.37CV 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 22.4568 2461274.9568 12.40 09:10:22.44 +62:33:04.4
152.41422 39.67223 galactic UMa Second-epoch detections are separated by 1.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:10:22.44 +62:33:04.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:10:22.44 +62:33:04.4: 13.36 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:10:22.44 +62:33:04.4: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 10 22.44 +62 33 04.4 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.40,0.05,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
target 20260822.4568 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.41 09:20:02.31 +64:09:13.5
149.96809 40.14200 galactic UMa Second-epoch detections are separated by 1.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:20:02.31 +64:09:13.5 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:20:02.31 +64:09:13.5: 13.35 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:20:02.31 +64:09:13.5: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 20 02.31 +64 09 13.5 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.45 10:16:12.41 +61:58:36.4
148.38222 46.74923 galactic UMa Second-epoch detections are separated by 2.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1051825224363817600 | 10:16:12.32 +61:59:10.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:16:12.41 +61:58:36.4: 13.36 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:16:12.41 +61:58:36.4: 13.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 16 12.41 +61 58 36.4 12.4 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 1051825224363817600,2461274.9568,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1051825224363817600 20260822.4568 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.23 10:19:57.73 +60:01:01.0
150.36466 48.25082 galactic UMa Second-epoch detections are separated by 2.1" and 7.1 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 | DocumentRef: VOTx1075146 | 10:19:57.73 +60:01:01.0 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.324+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:19:57.73 +60:01:01.0: 13.34 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:19:57.73 +60:01:01.0: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 19 57.73 +60 01 01.0 12.2 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
DocumentRef: VOTx1075146,2461274.9568,12.23,0.05,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
DocumentRef: VOTx1075146 20260822.4568 12.23CV 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 22.4568 2461274.9568 12.30 10:27:08.49 +62:22:09.7
146.78647 47.52643 galactic UMa Second-epoch detections are separated by 0.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:27:08.49 +62:22:09.7 (user input) | T | P | (position from user input) J-Ks=0.318+/-0.034 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:27:08.49 +62:22:09.7: 13.33 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:27:08.49 +62:22:09.7: 13.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 27 08.49 +62 22 09.7 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.30,0.05,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
target 20260822.4568 12.30CV 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 22.4568 2461274.9568 12.45 09:15:47.87 +63:31:49.6
150.94730 39.93023 galactic UMa Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:15:47.87 +63:31:49.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:15:47.87 +63:31:49.6: 13.35 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:15:47.87 +63:31:49.6: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 15 47.87 +63 31 49.6 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.35 09:59:39.78 +59:08:56.2
153.44114 46.51494 galactic UMa Second-epoch detections are separated by 1.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J149.9158+59.1490 | 09:59:39.78 +59:08:56.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.380+/-0.032 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:59:39.78 +59:08:56.2: 13.33 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:59:39.78 +59:08:56.2: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 59 39.78 +59 08 56.2 12.3 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
ATO J149.9158+59.1490,2461274.9568,12.35,0.05,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
ATO J149.9158+59.1490 20260822.4568 12.35CV 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 22.4568 2461274.9568 12.29 10:01:33.08 +58:44:06.4
153.80424 46.92556 galactic UMa Second-epoch detections are separated by 2.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1046880965387522048 | 10:01:33.08 +58:44:06.4 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G3 (LAMOST DR5) J-Ks=0.397+/-0.036 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:01:33.08 +58:44:06.4: 13.32 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:01:33.08 +58:44:06.4: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 01 33.08 +58 44 06.4 12.3 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
Large-amplitude variable Gaia DR2 1046880965387522048,2461274.9568,12.29,0.05,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 1046880965387522048 20260822.4568 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.27 10:25:54.31 +61:54:44.0
147.44959 47.69964 galactic UMa Second-epoch detections are separated by 2.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:25:54.31 +61:54:44.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:25:54.31 +61:54:44.0: 13.32 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:25:54.31 +61:54:44.0: 13.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 25 54.31 +61 54 44.0 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.27,0.05,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
target 20260822.4568 12.27CV 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 22.4568 2461274.9568 12.26 10:21:15.15 +60:56:22.7
149.10268 47.84472 galactic UMa Second-epoch detections are separated by 0.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:21:15.15 +60:56:22.7 (user input) | T | P | (position from user input) J-Ks=0.610+/-0.028 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:21:15.15 +60:56:22.7: 13.31 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:21:15.15 +60:56:22.7: 13.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 21 15.15 +60 56 22.7 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.40 10:29:20.30 +62:23:55.3
146.51295 47.70440 galactic UMa Second-epoch detections are separated by 1.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:29:20.30 +62:23:55.3 (user input) | T | P | (position from user input) J-Ks=0.546+/-0.028 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:29:20.30 +62:23:55.3: 13.32 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:29:20.30 +62:23:55.3: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 29 20.30 +62 23 55.3 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.40,0.05,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
target 20260822.4568 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.29 10:17:43.89 +60:38:42.3
149.83007 47.66550 galactic UMa Second-epoch detections are separated by 2.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:17:43.89 +60:38:42.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:17:43.89 +60:38:42.3: 13.29 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:17:43.89 +60:38:42.3: 13.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 17 43.89 +60 38 42.3 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.26 10:16:34.37 +61:08:33.6
149.34497 47.26563 galactic UMa Second-epoch detections are separated by 2.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:16:34.37 +61:08:33.6 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.032 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:16:34.37 +61:08:33.6: 13.31 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:16:34.37 +61:08:33.6: 13.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 16 34.37 +61 08 33.6 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.37 09:08:56.09 +65:12:52.3
149.23269 38.65521 galactic UMa Second-epoch detections are separated by 1.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:08:56.09 +65:12:52.3 (user input) | T | P | (position from user input) J-Ks=0.488+/-0.031 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:08:56.09 +65:12:52.3: 13.31 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:08:56.09 +65:12:52.3: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 08 56.09 +65 12 52.3 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.37,0.05,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
target 20260822.4568 12.37CV 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 22.4568 2461274.9568 12.26 09:58:36.71 +59:06:52.5
153.57725 46.41213 galactic UMa Second-epoch detections are separated by 0.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:58:36.71 +59:06:52.5 (user input) | T | P | (position from user input) J-Ks=0.504+/-0.035 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:58:36.71 +59:06:52.5: 13.29 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:58:36.71 +59:06:52.5: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 58 36.71 +59 06 52.5 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.29 09:59:52.04 +58:58:53.3
153.63783 46.61717 galactic UMa Second-epoch detections are separated by 1.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:59:52.04 +58:58:53.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.328+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:59:52.04 +58:58:53.3: 13.30 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:59:52.04 +58:58:53.3: 13.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 59 52.04 +58 58 53.3 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.38 09:21:17.46 +64:22:14.5
149.63809 40.18623 galactic UMa Second-epoch detections are separated by 1.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:21:17.46 +64:22:14.5 (user input) | T | P | (position from user input) J-Ks=0.374+/-0.028 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:21:17.46 +64:22:14.5: 13.29 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:21:17.46 +64:22:14.5: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 21 17.46 +64 22 14.5 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.38,0.05,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
target 20260822.4568 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.24 10:08:25.45 +61:01:15.9
150.29170 46.51296 galactic UMa Second-epoch detections are separated by 0.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx1894439 | 10:08:25.45 +61:01:15.9 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:08:25.45 +61:01:15.9: 13.30 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:08:25.45 +61:01:15.9: 13.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 08 25.45 +61 01 15.9 12.2 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
DocumentRef: VOTx1894439,2461274.9568,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx1894439 20260822.4568 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.39 09:15:38.54 +64:21:11.7
149.95296 39.62472 galactic UMa Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:15:38.54 +64:21:11.7 (user input) | T | P | (position from user input) J-Ks=0.322+/-0.029 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:15:38.54 +64:21:11.7: 13.28 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:15:38.54 +64:21:11.7: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 15 38.54 +64 21 11.7 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.30 09:57:52.91 +58:24:03.5
154.56114 46.65730 galactic UMa Second-epoch detections are separated by 2.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:57:52.91 +58:24:03.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:57:52.91 +58:24:03.5: 13.28 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:57:52.91 +58:24:03.5: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 57 52.91 +58 24 03.5 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.30,0.05,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
target 20260822.4568 12.30CV 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 22.4568 2461274.9568 12.22 09:57:29.91 +58:33:56.7
154.38074 46.53774 galactic UMa Second-epoch detections are separated by 0.4" and 7.0 pix
The object was found in VSX 2" Gaia DR3 1046512319754626816
Type: ROT
# Max. Min./Amp. JD0 Period
13.080 G 13.110 G G
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:57:29.91 +58:33:56.7: 13.27 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:57:29.91 +58:33:56.7: 13.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 57 29.91 +58 33 56.7 12.2 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 1046512319754626816,2461274.9568,12.22,0.05,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 1046512319754626816 20260822.4568 12.22CV 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 22.4568 2461274.9568 12.25 10:17:29.85 +61:43:41.3
148.54844 47.01772 galactic UMa Second-epoch detections are separated by 0.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:17:29.85 +61:43:41.3 (user input) | T | P | (position from user input) J-Ks=0.619+/-0.033 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:17:29.85 +61:43:41.3: 13.28 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:17:29.85 +61:43:41.3: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 17 29.85 +61 43 41.3 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.25,0.05,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
target 20260822.4568 12.25CV 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 22.4568 2461274.9568 12.29 09:57:12.38 +59:40:13.4
152.98916 45.99349 galactic UMa Second-epoch detections are separated by 0.9" and 6.9 pix
The object was found in VSX 1" ASASSN-V J095712.33+594014.0
Type: VAR
# Max. Min./Amp. JD0 Period
13.790 g Y 0.160 g 2458612.70700 1.378500000000
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:57:12.38 +59:40:13.4: 13.27 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:57:12.38 +59:40:13.4: 13.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 57 12.38 +59 40 13.4 12.3 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
ASASSN-V J095712.33+594014.0,2461274.9568,12.29,0.05,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 J095712.33+594014.0 20260822.4568 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.23 10:18:02.30 +60:14:24.3
150.29405 47.92686 galactic UMa Second-epoch detections are separated by 2.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx1917776 | 10:18:02.30 +60:14:24.3 (user input) | (GCVS) | (GCVS) | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:18:02.30 +60:14:24.3: 13.27 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:18:02.30 +60:14:24.3: 13.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 18 02.30 +60 14 24.3 12.2 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
DocumentRef: VOTx1917776,2461274.9568,12.23,0.05,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
DocumentRef: VOTx1917776 20260822.4568 12.23CV 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 22.4568 2461274.9568 12.38 09:18:25.57 +64:42:41.2
149.37761 39.77265 galactic UMa Second-epoch detections are separated by 1.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:18:25.57 +64:42:41.2 (user input) | T | P | (position from user input) J-Ks=0.351+/-0.030 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:18:25.57 +64:42:41.2: 13.27 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:18:25.57 +64:42:41.2: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 18 25.57 +64 42 41.2 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.38,0.05,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
target 20260822.4568 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.24 10:27:31.05 +63:04:43.3
145.93815 47.10897 galactic UMa Second-epoch detections are separated by 0.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:27:31.05 +63:04:43.3 (user input) | T | P | (position from user input) J-Ks=0.581+/-0.032 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:27:31.05 +63:04:43.3: 13.27 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:27:31.05 +63:04:43.3: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 27 31.05 +63 04 43.3 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.34 10:16:15.69 +61:21:27.8
149.11708 47.11179 galactic UMa Second-epoch detections are separated by 1.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:16:15.69 +61:21:27.8 (user input) | T | P | (position from user input) J-Ks=0.263+/-0.033 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:16:15.69 +61:21:27.8: 13.28 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:16:15.69 +61:21:27.8: 13.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 16 15.69 +61 21 27.8 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.29 10:06:16.40 +60:17:19.1
151.39977 46.67462 galactic UMa Second-epoch detections are separated by 1.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:06:16.40 +60:17:19.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:06:16.40 +60:17:19.1: 13.26 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:06:16.40 +60:17:19.1: 13.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 06 16.40 +60 17 19.1 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.37 09:13:33.47 +63:26:22.6
151.16968 39.72631 galactic UMa Second-epoch detections are separated by 2.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:13:33.47 +63:26:22.6 (user input) | T | P | (position from user input) J-Ks=0.462+/-0.031 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:13:33.47 +63:26:22.6: 13.27 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:13:33.47 +63:26:22.6: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 13 33.47 +63 26 22.6 12.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.37,0.05,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
target 20260822.4568 12.37CV 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 22.4568 2461274.9568 12.26 10:10:49.67 +59:25:25.9
152.04715 47.61315 galactic UMa Second-epoch detections are separated by 2.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:49.67 +59:25:25.9 (user input) | T | P | (position from user input) J-Ks=0.982+/-0.028 (M)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:10:49.67 +59:25:25.9: 13.27 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:10:49.67 +59:25:25.9: 13.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 10 49.67 +59 25 25.9 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.31 10:20:35.71 +62:06:21.9
147.78462 47.08784 galactic UMa Second-epoch detections are separated by 1.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:20:35.71 +62:06:21.9 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.032 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:20:35.71 +62:06:21.9: 13.27 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:20:35.71 +62:06:21.9: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 20 35.71 +62 06 21.9 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.31,0.05,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
target 20260822.4568 12.31CV 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 22.4568 2461274.9568 12.30 10:10:31.95 +60:55:20.5
150.21164 46.78154 galactic UMa Second-epoch detections are separated by 1.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:31.95 +60:55:20.5 (user input) | T | P | (position from user input) J-Ks=0.499+/-0.032 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:10:31.95 +60:55:20.5: 13.25 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:10:31.95 +60:55:20.5: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 10 31.95 +60 55 20.5 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.30,0.05,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
target 20260822.4568 12.30CV 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 22.4568 2461274.9568 12.21 09:59:57.05 +59:24:09.5
153.09169 46.42668 galactic UMa Second-epoch detections are separated by 2.9" and 7.4 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 J149.9866+59.4026 | 09:59:57.05 +59:24:09.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.369+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:59:57.05 +59:24:09.5: 13.24 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:59:57.05 +59:24:09.5: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 59 57.05 +59 24 09.5 12.2 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 J149.9866+59.4026,2461274.9568,12.21,0.05,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
ATO J149.9866+59.4026 20260822.4568 12.21CV 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 22.4568 2461274.9568 12.33 09:14:34.67 +62:46:18.7
151.93971 40.05820 galactic UMa Second-epoch detections are separated by 0.8" and 6.8 pix
The object was found in VSX 5" Gaia DR3 1043287486510907264
Type: ROT
# Max. Min./Amp. JD0 Period
12.420 G 12.460 G M
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:14:34.67 +62:46:18.7: 13.26 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:14:34.67 +62:46:18.7: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 14 34.67 +62 46 18.7 12.3 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 1043287486510907264,2461274.9568,12.33,0.05,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 1043287486510907264 20260822.4568 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 22.4568 2461274.9568 12.35 09:13:47.07 +63:41:47.8
150.84431 39.66305 galactic UMa Second-epoch detections are separated by 0.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:13:47.07 +63:41:47.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:13:47.07 +63:41:47.8: 13.24 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:13:47.07 +63:41:47.8: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 13 47.07 +63 41 47.8 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.35,0.05,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
target 20260822.4568 12.35CV 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 22.4568 2461274.9568 12.23 10:41:02.20 +63:31:05.1
143.94900 47.94256 galactic UMa Second-epoch detections are separated by 1.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:41:02.20 +63:31:05.1 (user input) | T | P | (position from user input) J-Ks=0.482+/-0.028 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:41:02.20 +63:31:05.1: 13.24 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:41:02.20 +63:31:05.1: 13.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 41 02.20 +63 31 05.1 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.23,0.05,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
target 20260822.4568 12.23CV 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 22.4568 2461274.9568 12.24 10:47:07.03 +62:39:22.2
144.13738 49.03829 galactic UMa Second-epoch detections are separated by 1.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1055003023421636096 | 10:47:07.03 +62:39:22.2 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:47:07.03 +62:39:22.2: 13.24 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:47:07.03 +62:39:22.2: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 47 07.03 +62 39 22.2 12.2 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
Large-amplitude variable Gaia DR2 1055003023421636096,2461274.9568,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1055003023421636096 20260822.4568 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.18 10:01:48.91 +59:19:34.4
153.02290 46.67165 galactic UMa Second-epoch detections are separated by 2.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:01:48.91 +59:19:34.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:01:48.91 +59:19:34.4: 13.22 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:01:48.91 +59:19:34.4: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 01 48.91 +59 19 34.4 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.18,0.05,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
target 20260822.4568 12.18CV 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 22.4568 2461274.9568 12.33 10:06:27.02 +59:31:55.2
152.33380 47.08129 galactic UMa Second-epoch detections are separated by 3.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:06:27.02 +59:31:55.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:06:27.02 +59:31:55.2: 13.22 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:06:27.02 +59:31:55.2: 13.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 06 27.02 +59 31 55.2 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 22.4568 2461274.9568 12.27 10:27:21.73 +62:06:51.9
147.05631 47.70690 galactic UMa Second-epoch detections are separated by 2.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:27:21.73 +62:06:51.9 (user input) | T | P | (position from user input) J-Ks=0.236+/-0.038 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:27:21.73 +62:06:51.9: 13.26 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:27:21.73 +62:06:51.9: 13.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 27 21.73 +62 06 51.9 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.27,0.05,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
target 20260822.4568 12.27CV 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 22.4568 2461274.9568 12.18 10:19:49.79 +61:37:46.1
148.42690 47.29955 galactic UMa Second-epoch detections are separated by 2.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:19:49.79 +61:37:46.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:19:49.79 +61:37:46.1: 13.22 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:19:49.79 +61:37:46.1: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 19 49.79 +61 37 46.1 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.18,0.05,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
target 20260822.4568 12.18CV 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 22.4568 2461274.9568 12.31 10:29:23.58 +62:36:56.6
146.25980 47.57007 galactic UMa Second-epoch detections are separated by 1.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:29:23.58 +62:36:56.6 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.030 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:29:23.58 +62:36:56.6: 13.21 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:29:23.58 +62:36:56.6: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 29 23.58 +62 36 56.6 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.31,0.05,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
target 20260822.4568 12.31CV 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 22.4568 2461274.9568 12.23 10:18:05.01 +59:48:06.0
150.83105 48.17864 galactic UMa Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:18:05.01 +59:48:06.0 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.031 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:18:05.01 +59:48:06.0: 13.20 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:18:05.01 +59:48:06.0: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 18 05.01 +59 48 06.0 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.23,0.05,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
target 20260822.4568 12.23CV 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 22.4568 2461274.9568 12.25 10:03:46.88 +59:09:42.3
153.05355 46.97131 galactic UMa Second-epoch detections are separated by 1.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:03:46.88 +59:09:42.3 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.469+/-0.027 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:03:46.88 +59:09:42.3: 13.21 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:03:46.88 +59:09:42.3: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 03 46.88 +59 09 42.3 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.25,0.05,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
target 20260822.4568 12.25CV 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 22.4568 2461274.9568 12.23 10:37:03.90 +63:58:35.7
143.91002 47.30821 galactic UMa Second-epoch detections are separated by 0.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:37:03.90 +63:58:35.7 (user input) | T | P | (position from user input) J-Ks=0.722+/-0.028 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:37:03.90 +63:58:35.7: 13.21 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:37:03.90 +63:58:35.7: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 37 03.90 +63 58 35.7 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.23,0.05,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
target 20260822.4568 12.23CV 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 22.4568 2461274.9568 12.25 10:02:24.15 +59:08:11.8
153.21183 46.82925 galactic UMa Second-epoch detections are separated by 1.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:02:24.15 +59:08:11.8 (user input) | T | P | (position from user input) J-Ks=0.580+/-0.028 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:02:24.15 +59:08:11.8: 13.19 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:02:24.15 +59:08:11.8: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 02 24.15 +59 08 11.8 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.25,0.05,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
target 20260822.4568 12.25CV 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 22.4568 2461274.9568 12.24 10:26:43.74 +61:36:14.2
147.71983 47.96727 galactic UMa Second-epoch detections are separated by 1.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:26:43.74 +61:36:14.2 (user input) | T | P | (position from user input) J-Ks=0.556+/-0.030 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:26:43.74 +61:36:14.2: 13.19 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:26:43.74 +61:36:14.2: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 26 43.74 +61 36 14.2 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.10 10:27:00.03 +61:15:52.5
148.08897 48.20267 galactic UMa Second-epoch detections are separated by 0.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:27:00.03 +61:15:52.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:27:00.03 +61:15:52.5: 13.18 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:27:00.03 +61:15:52.5: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 27 00.03 +61 15 52.5 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.13 10:06:44.77 +60:42:28.8
150.83474 46.50585 galactic UMa Second-epoch detections are separated by 0.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:06:44.77 +60:42:28.8 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.062 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:06:44.77 +60:42:28.8: 13.17 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:06:44.77 +60:42:28.8: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 06 44.77 +60 42 28.8 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.13CV 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 22.4568 2461274.9568 12.19 10:12:38.50 +61:07:06.7
149.76689 46.88725 galactic UMa Second-epoch detections are separated by 0.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:38.50 +61:07:06.7 (user input) | T | P | (position from user input) J-Ks=0.437+/-0.031 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:12:38.50 +61:07:06.7: 13.16 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:12:38.50 +61:07:06.7: 13.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 12 38.50 +61 07 06.7 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.19,0.05,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
target 20260822.4568 12.19CV 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 22.4568 2461274.9568 12.11 10:06:16.55 +59:51:03.8
151.94770 46.89985 galactic UMa Second-epoch detections are separated by 2.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:06:16.55 +59:51:03.8 (user input) | T | P | (position from user input) J-Ks=0.326+/-0.027 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:06:16.55 +59:51:03.8: 13.18 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:06:16.55 +59:51:03.8: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 06 16.55 +59 51 03.8 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.11,0.05,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
target 20260822.4568 12.11CV 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 22.4568 2461274.9568 12.19 10:05:21.03 +59:54:08.2
151.96973 46.77386 galactic UMa Second-epoch detections are separated by 3.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:05:21.03 +59:54:08.2 (user input) | T | P | (position from user input) J-Ks=0.356+/-0.027 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:05:21.03 +59:54:08.2: 13.17 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:05:21.03 +59:54:08.2: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 22.4568* 10 05 21.03 +59 54 08.2 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.19,0.05,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
target 20260822.4568 12.19CV 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 22.4568 2461274.9568 12.30 10:26:55.65 +61:08:00.0
148.25233 48.27660 galactic UMa Second-epoch detections are separated by 1.4" and 7.1 pix
The object was found in VSX 1" Gaia DR3 1048681312599357440
Type: ROT
# Max. Min./Amp. JD0 Period
12.940 G 13.000 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:26:55.65 +61:08:00.0: 13.18 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:26:55.65 +61:08:00.0: 13.30 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 26 55.65 +61 08 00.0 12.3 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 1048681312599357440,2461274.9568,12.30,0.05,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 1048681312599357440 20260822.4568 12.30CV 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 22.4568 2461274.9568 12.18 09:52:08.82 +57:15:33.6
156.53868 46.46467 galactic UMa Second-epoch detections are separated by 2.3" and 7.3 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 | DocumentRef: VOTx3798303 | 09:52:08.82 +57:15:33.6 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.382+/-0.034 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:52:08.82 +57:15:33.6: 13.15 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:52:08.82 +57:15:33.6: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 52 08.82 +57 15 33.6 12.2 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
DocumentRef: VOTx3798303,2461274.9568,12.18,0.05,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
DocumentRef: VOTx3798303 20260822.4568 12.18CV 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 22.4568 2461274.9568 12.11 10:04:08.19 +58:18:37.8
154.11594 47.42484 galactic UMa Second-epoch detections are separated by 1.8" and 7.1 pix
The object was found in VSX 2" Gaia DR3 1046620582994747776
Type: ROT
# Max. Min./Amp. JD0 Period
12.890 G 12.930 G G
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:04:08.19 +58:18:37.8: 13.17 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:04:08.19 +58:18:37.8: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 04 08.19 +58 18 37.8 12.1 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 1046620582994747776,2461274.9568,12.11,0.05,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 1046620582994747776 20260822.4568 12.11CV 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 22.4568 2461274.9568 12.13 10:20:55.01 +61:30:55.6
148.44913 47.47133 galactic UMa Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:20:55.01 +61:30:55.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:20:55.01 +61:30:55.6: 13.15 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:20:55.01 +61:30:55.6: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 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 22.4568* 10 20 55.01 +61 30 55.6 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.13CV 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 22.4568 2461274.9568 12.18 10:08:24.15 +59:15:31.6
152.49354 47.43432 galactic UMa Second-epoch detections are separated by 1.7" and 7.2 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 | DocumentRef: VOTx4103909 | 10:08:24.15 +59:15:31.6 (user input) | (GCVS) | (GCVS) | (position from user input) SpType: F8 (LAMOST DR5)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:08:24.15 +59:15:31.6: 13.17 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:08:24.15 +59:15:31.6: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 08 24.15 +59 15 31.6 12.2 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
DocumentRef: VOTx4103909,2461274.9568,12.18,0.05,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
DocumentRef: VOTx4103909 20260822.4568 12.18CV 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 22.4568 2461274.9568 12.28 10:34:12.40 +63:20:41.7
144.91341 47.50404 galactic UMa Second-epoch detections are separated by 0.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:34:12.40 +63:20:41.7 (user input) | T | P | (position from user input) J-Ks=0.386+/-0.029 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:34:12.40 +63:20:41.7: 13.16 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:34:12.40 +63:20:41.7: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 34 12.40 +63 20 41.7 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.22 09:10:52.85 +62:18:17.8
152.69488 39.80456 galactic UMa Second-epoch detections are separated by 1.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:10:52.85 +62:18:17.8 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.032 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:10:52.85 +62:18:17.8: 13.16 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:10:52.85 +62:18:17.8: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 10 52.85 +62 18 17.8 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.22,0.05,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
target 20260822.4568 12.22CV 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 22.4568 2461274.9568 12.18 10:16:48.91 +61:27:26.6
148.94131 47.10866 galactic UMa Second-epoch detections are separated by 1.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:16:48.91 +61:27:26.6 (user input) | T | P | (position from user input) J-Ks=0.465+/-0.033 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:16:48.91 +61:27:26.6: 13.14 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:16:48.91 +61:27:26.6: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 16 48.91 +61 27 26.6 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.18,0.05,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
target 20260822.4568 12.18CV 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 22.4568 2461274.9568 12.20 10:25:21.16 +60:56:52.2
148.64781 48.23894 galactic UMa Second-epoch detections are separated by 1.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx584553 | 10:25:21.16 +60:56:52.2 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.539+/-0.048 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:25:21.16 +60:56:52.2: 13.15 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:25:21.16 +60:56:52.2: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.18 +/- 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 22.4568* 10 25 21.16 +60 56 52.2 12.2 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
DocumentRef: VOTx584553,2461274.9568,12.20,0.05,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
DocumentRef: VOTx584553 20260822.4568 12.20CV 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 22.4568 2461274.9568 12.14 10:30:11.78 +63:08:48.5
145.57368 47.29618 galactic UMa Second-epoch detections are separated by 1.4" and 6.8 pix
The object was found in VSX 2" Gaia DR3 1052274894555820544
Type: ROT
# Max. Min./Amp. JD0 Period
12.860 G 12.900 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:30:11.78 +63:08:48.5: 13.13 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:30:11.78 +63:08:48.5: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 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 22.4568* 10 30 11.78 +63 08 48.5 12.1 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 1052274894555820544,2461274.9568,12.14,0.05,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 1052274894555820544 20260822.4568 12.14CV 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 22.4568 2461274.9568 12.16 09:57:57.86 +57:18:25.6
155.98661 47.15558 galactic UMa Second-epoch detections are separated by 1.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx612012 | 09:57:57.86 +57:18:25.6 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.512+/-0.032 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:57:57.86 +57:18:25.6: 13.12 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:57:57.86 +57:18:25.6: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 57 57.86 +57 18 25.6 12.2 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
DocumentRef: VOTx612012,2461274.9568,12.16,0.05,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
DocumentRef: VOTx612012 20260822.4568 12.16CV 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 22.4568 2461274.9568 12.10 10:16:57.68 +60:44:25.6
149.79340 47.53373 galactic UMa Second-epoch detections are separated by 0.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:16:57.68 +60:44:25.6 (user input) | T | P | (position from user input) J-Ks=0.398+/-0.030 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:16:57.68 +60:44:25.6: 13.13 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:16:57.68 +60:44:25.6: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.15 +/- 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 22.4568* 10 16 57.68 +60 44 25.6 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.18 09:14:54.25 +64:11:42.9
150.18160 39.60578 galactic UMa Second-epoch detections are separated by 1.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx725975 | 09:14:54.25 +64:11:42.9 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.653+/-0.027 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:14:54.25 +64:11:42.9: 13.11 +/- 0.03 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:14:54.25 +64:11:42.9: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 14 54.25 +64 11 42.9 12.2 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
DocumentRef: VOTx725975,2461274.9568,12.18,0.05,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
DocumentRef: VOTx725975 20260822.4568 12.18CV 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 22.4568 2461274.9568 12.20 10:18:46.00 +62:03:32.2
148.02738 46.94419 galactic UMa Second-epoch detections are separated by 1.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:18:46.00 +62:03:32.2 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.031 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:18:46.00 +62:03:32.2: 13.11 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:18:46.00 +62:03:32.2: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 22.4568* 10 18 46.00 +62 03 32.2 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.20,0.05,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
target 20260822.4568 12.20CV 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 22.4568 2461274.9568 12.15 10:25:52.64 +61:24:47.5
148.03774 48.00505 galactic UMa Second-epoch detections are separated by 2.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:25:52.64 +61:24:47.5 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:25:52.64 +61:24:47.5: 13.11 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:25:52.64 +61:24:47.5: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 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 22.4568* 10 25 52.64 +61 24 47.5 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.15,0.05,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
target 20260822.4568 12.15CV 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 22.4568 2461274.9568 12.16 10:14:37.24 +60:00:22.3
150.93661 47.70400 galactic UMa Second-epoch detections are separated by 2.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx766370 | 10:14:37.24 +60:00:22.3 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.421+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:14:37.24 +60:00:22.3: 13.10 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:14:37.24 +60:00:22.3: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 14 37.24 +60 00 22.3 12.2 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
DocumentRef: VOTx766370,2461274.9568,12.16,0.05,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
DocumentRef: VOTx766370 20260822.4568 12.16CV 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 22.4568 2461274.9568 11.99 10:15:56.25 +59:41:47.2
151.18687 48.01237 galactic UMa Second-epoch detections are separated by 0.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:15:56.25 +59:41:47.2 (user input) | T | P | (position from user input) J-Ks=0.623+/-0.032 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:15:56.25 +59:41:47.2: 13.11 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:15:56.25 +59:41:47.2: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 15 56.25 +59 41 47.2 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.16 09:57:08.65 +58:53:29.2
153.99078 46.34803 galactic UMa Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:57:08.65 +58:53:29.2 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.307+/-0.034 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:57:08.65 +58:53:29.2: 13.10 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:57:08.65 +58:53:29.2: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 57 08.65 +58 53 29.2 12.2 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.16,0.05,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
target 20260822.4568 12.16CV 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 22.4568 2461274.9568 12.11 10:21:28.39 +60:30:27.4
149.60168 48.12006 galactic UMa Second-epoch detections are separated by 0.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:21:28.39 +60:30:27.4 (user input) | T | P | (position from user input) J-Ks=0.323+/-0.031 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:21:28.39 +60:30:27.4: 13.06 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:21:28.39 +60:30:27.4: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 21 28.39 +60 30 27.4 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.11,0.05,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
target 20260822.4568 12.11CV 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 22.4568 2461274.9568 12.12 10:18:44.24 +61:57:16.8
148.15356 47.00313 galactic UMa Second-epoch detections are separated by 1.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:18:44.24 +61:57:16.8 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:18:44.24 +61:57:16.8: 13.04 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:18:44.24 +61:57:16.8: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 18 44.24 +61 57 16.8 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.13 10:07:05.17 +58:02:21.7
154.18842 47.89637 galactic UMa Second-epoch detections are separated by 2.1" and 7.0 pix
The object was found in VSX 3" Gaia DR3 1046557532874852608
Type: ROT
# Max. Min./Amp. JD0 Period
12.660 G 12.690 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:07:05.17 +58:02:21.7: 13.02 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:07:05.17 +58:02:21.7: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 07 05.17 +58 02 21.7 12.1 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 1046557532874852608,2461274.9568,12.13,0.05,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 1046557532874852608 20260822.4568 12.13CV 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 22.4568 2461274.9568 12.01 09:55:58.76 +57:53:34.4
155.38681 46.65967 galactic UMa Second-epoch detections are separated by 0.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:55:58.76 +57:53:34.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.489+/-0.032 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:55:58.76 +57:53:34.4: 13.03 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:55:58.76 +57:53:34.4: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 22.4568* 09 55 58.76 +57 53 34.4 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.01CV 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 22.4568 2461274.9568 12.04 09:56:36.25 +57:30:28.6
155.83907 46.90306 galactic UMa Second-epoch detections are separated by 2.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:56:36.25 +57:30:28.6 (user input) | T | P | (position from user input) J-Ks=0.680+/-0.035 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:56:36.25 +57:30:28.6: 13.03 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:56:36.25 +57:30:28.6: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 22.4568* 09 56 36.25 +57 30 28.6 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.04CV 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 22.4568 2461274.9568 12.09 10:35:25.53 +63:09:04.7
144.98977 47.73566 galactic UMa Second-epoch detections are separated by 2.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:35:25.53 +63:09:04.7 (user input) | T | P | (position from user input) J-Ks=0.398+/-0.028 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:35:25.53 +63:09:04.7: 13.02 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:35:25.53 +63:09:04.7: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 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 22.4568* 10 35 25.53 +63 09 04.7 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.06 09:58:53.69 +59:23:23.5
153.20060 46.31452 galactic UMa Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:58:53.69 +59:23:23.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.506+/-0.034 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:58:53.69 +59:23:23.5: 13.02 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:58:53.69 +59:23:23.5: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 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 22.4568* 09 58 53.69 +59 23 23.5 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.06,0.05,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
target 20260822.4568 12.06CV 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 22.4568 2461274.9568 12.15 10:23:42.01 +61:00:02.0
148.76599 48.04726 galactic UMa Second-epoch detections are separated by 1.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx778732 | 10:23:42.01 +61:00:02.0 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.826+/-0.033 (M)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:23:42.01 +61:00:02.0: 13.02 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:23:42.01 +61:00:02.0: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 23 42.01 +61 00 02.0 12.2 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
DocumentRef: VOTx778732,2461274.9568,12.15,0.05,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
DocumentRef: VOTx778732 20260822.4568 12.15CV 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 22.4568 2461274.9568 12.03 09:55:49.10 +58:12:57.3
154.97865 46.49814 galactic UMa Second-epoch detections are separated by 0.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:55:49.10 +58:12:57.3 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.391+/-0.030 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:55:49.10 +58:12:57.3: 12.99 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:55:49.10 +58:12:57.3: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 22.4568* 09 55 49.10 +58 12 57.3 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.03CV 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 22.4568 2461274.9568 12.05 10:18:31.41 +60:59:24.5
149.32887 47.54636 galactic UMa Second-epoch detections are separated by 2.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:18:31.41 +60:59:24.5 (user input) | T | P | (position from user input) J-Ks=0.517+/-0.031 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:18:31.41 +60:59:24.5: 12.99 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:18:31.41 +60:59:24.5: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 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 22.4568* 10 18 31.41 +60 59 24.5 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.05CV 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 22.4568 2461274.9568 12.11 10:11:49.64 +60:47:49.0
150.23961 46.98207 galactic UMa Second-epoch detections are separated by 1.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:49.64 +60:47:49.0 (user input) | T | P | (position from user input) J-Ks=0.323+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:11:49.64 +60:47:49.0: 12.98 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:11:49.64 +60:47:49.0: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 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 22.4568* 10 11 49.64 +60 47 49.0 12.1 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.11,0.05,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
target 20260822.4568 12.11CV 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 22.4568 2461274.9568 12.03 10:03:14.12 +59:34:59.3
152.56755 46.70321 galactic UMa Second-epoch detections are separated by 3.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:03:14.12 +59:34:59.3 (user input) | T | P | (position from user input) J-Ks=0.278+/-0.028 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:03:14.12 +59:34:59.3: 12.98 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:03:14.12 +59:34:59.3: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 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 22.4568* 10 03 14.12 +59 34 59.3 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.03CV 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 22.4568 2461274.9568 12.04 10:11:35.54 +61:19:40.9
149.61445 46.66603 galactic UMa Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:11:35.54 +61:19:40.9 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.032 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:11:35.54 +61:19:40.9: 12.97 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:11:35.54 +61:19:40.9: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 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 22.4568* 10 11 35.54 +61 19 40.9 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.04CV 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 22.4568 2461274.9568 12.01 10:14:31.42 +59:43:49.7
151.29003 47.84457 galactic UMa Second-epoch detections are separated by 2.3" and 6.6 pix
The object was found in VSX 1" Gaia DR3 1048494636141255168
Type: ROT
# Max. Min./Amp. JD0 Period
12.580 G 12.600 G 10.356200000000 K
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:14:31.42 +59:43:49.7: 12.95 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:14:31.42 +59:43:49.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 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 22.4568* 10 14 31.42 +59 43 49.7 12.0 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 1048494636141255168,2461274.9568,12.01,0.05,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 1048494636141255168 20260822.4568 12.01CV 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 22.4568 2461274.9568 12.00 10:23:57.27 +60:51:54.5
148.90050 48.15319 galactic UMa Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:23:57.27 +60:51:54.5 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.033 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:23:57.27 +60:51:54.5: 12.93 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:23:57.27 +60:51:54.5: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 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 22.4568* 10 23 57.27 +60 51 54.5 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 22.4568 2461274.9568 11.97 10:00:30.51 +58:38:27.4
154.01931 46.85059 galactic UMa Second-epoch detections are separated by 1.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:00:30.51 +58:38:27.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.340+/-0.034 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:00:30.51 +58:38:27.4: 12.91 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:00:30.51 +58:38:27.4: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 00 30.51 +58 38 27.4 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 11.97CV 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 22.4568 2461274.9568 11.97 09:57:59.53 +59:22:39.0
153.29469 46.21897 galactic UMa Second-epoch detections are separated by 0.4" and 6.9 pix
The object was found in VSX 1" ASASSN-V J095759.51+592239.5
Type: VAR
# Max. Min./Amp. JD0 Period
13.680 g Y 0.190 g 2458053.00200 0.999361000000
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:57:59.53 +59:22:39.0: 12.90 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:57:59.53 +59:22:39.0: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 57 59.53 +59 22 39.0 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J095759.51+592239.5,2461274.9568,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J095759.51+592239.5 20260822.4568 11.97CV 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 22.4568 2461274.9568 11.95 10:15:15.66 +60:29:19.5
150.27530 47.50312 galactic UMa Second-epoch detections are separated by 1.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:15:15.66 +60:29:19.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:15:15.66 +60:29:19.5: 12.89 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:15:15.66 +60:29:19.5: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 22.4568* 10 15 15.66 +60 29 19.5 11.9 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,11.95,0.05,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
target 20260822.4568 11.95CV 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 22.4568 2461274.9568 11.97 10:25:43.74 +63:09:53.5
146.02958 46.89826 galactic UMa Second-epoch detections are separated by 0.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:25:43.74 +63:09:53.5 (user input) | T | P | (position from user input) J-Ks=0.803+/-0.037 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:25:43.74 +63:09:53.5: 12.88 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:25:43.74 +63:09:53.5: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 22.4568* 10 25 43.74 +63 09 53.5 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 11.97CV 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 22.4568 2461274.9568 11.96 10:04:53.11 +59:53:18.4
152.03030 46.73056 galactic UMa Second-epoch detections are separated by 0.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:04:53.11 +59:53:18.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:04:53.11 +59:53:18.4: 12.87 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:04:53.11 +59:53:18.4: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 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 22.4568* 10 04 53.11 +59 53 18.4 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 11.96CV 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 22.4568 2461274.9568 11.96 09:58:37.16 +58:44:06.8
154.06444 46.58949 galactic UMa Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:58:37.16 +58:44:06.8 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.493+/-0.034 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:58:37.16 +58:44:06.8: 12.87 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:58:37.16 +58:44:06.8: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 58 37.16 +58 44 06.8 12.0 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 11.96CV 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 22.4568 2461274.9568 11.84 10:09:14.07 +60:24:51.6
150.96298 46.92057 galactic UMa Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:09:14.07 +60:24:51.6 (user input) | T | P | (position from user input) J-Ks=0.709+/-0.033 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:09:14.07 +60:24:51.6: 12.83 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:09:14.07 +60:24:51.6: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 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 22.4568* 10 09 14.07 +60 24 51.6 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,11.84,0.05,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
target 20260822.4568 11.84CV 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 22.4568 2461274.9568 11.85 10:08:00.96 +60:37:32.6
150.81727 46.68139 galactic UMa Second-epoch detections are separated by 1.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:08:00.96 +60:37:32.6 (user input) | T | P | (position from user input) J-Ks=0.559+/-0.035 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:08:00.96 +60:37:32.6: 12.76 +/- 0.01 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:08:00.96 +60:37:32.6: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 22.4568* 10 08 00.96 +60 37 32.6 11.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 11.85CV 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 22.4568 2461274.9568 11.80 10:08:15.86 +59:55:29.8
151.66630 47.07539 galactic UMa Second-epoch detections are separated by 2.9" and 7.3 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 | DocumentRef: VOTx1669107 | 10:08:15.86 +59:55:29.8 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.630+/-0.028 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:08:15.86 +59:55:29.8: 12.75 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:08:15.86 +59:55:29.8: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 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 22.4568* 10 08 15.86 +59 55 29.8 11.8 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
DocumentRef: VOTx1669107,2461274.9568,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx1669107 20260822.4568 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 11.82 09:47:28.49 +57:33:32.3
156.51122 45.76808 galactic UMa Second-epoch detections are separated by 1.1" and 6.8 pix
The object was found in VSX 1" Gaia DR3 1025337546869856256
Type: ROT
# Max. Min./Amp. JD0 Period
12.380 G 12.420 G K
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:47:28.49 +57:33:32.3: 12.74 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:47:28.49 +57:33:32.3: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 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 22.4568* 09 47 28.49 +57 33 32.3 11.8 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 1025337546869856256,2461274.9568,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1025337546869856256 20260822.4568 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 11.76 10:17:31.60 +60:25:32.1
150.11974 47.76959 galactic UMa Second-epoch detections are separated by 0.2" and 7.0 pix
The object was found in VSX 1" Gaia DR3 1048552184406353280
Type: ROT
# Max. Min./Amp. JD0 Period
12.450 G 12.490 G G
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:17:31.60 +60:25:32.1: 12.68 +/- 0.01 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:17:31.60 +60:25:32.1: 12.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 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 22.4568* 10 17 31.60 +60 25 32.1 11.8 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 1048552184406353280,2461274.9568,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1048552184406353280 20260822.4568 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 11.59 10:21:20.89 +60:12:30.3
149.98013 48.28170 galactic UMa Second-epoch detections are separated by 0.8" and 7.1 pix
The object was found in VSX 0" NSVS 2557361
Type: EW
# Max. Min./Amp. JD0 Period
12.490 R1 Y 0.590 R1 0.395355700000
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:21:20.89 +60:12:30.3: 12.39 +/- 0.01 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:21:20.89 +60:12:30.3: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 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 22.4568* 10 21 20.89 +60 12 30.3 11.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2557361,2461274.9568,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 2557361 20260822.4568 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4568 2461274.9568 12.64 09:21:32.11 +64:07:07.1
149.93041 40.30646 galactic UMa Second-epoch detections are separated by 1.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:21:32.11 +64:07:07.1 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.030 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 09:21:32.11 +64:07:07.1: 13.87 +/- 0.05 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 09:21:32.11 +64:07:07.1: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 09 21 32.11 +64 07 07.1 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.64,0.05,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
target 20260822.4568 12.64CV 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 22.4568 2461274.9568 12.64 10:16:33.89 +61:41:53.2
148.67836 46.94524 galactic UMa Second-epoch detections are separated by 1.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:16:33.89 +61:41:53.2 (user input) | T | P | (position from user input) J-Ks=0.805+/-0.030 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:16:33.89 +61:41:53.2: 13.84 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:16:33.89 +61:41:53.2: 13.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 16 33.89 +61 41 53.2 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.64,0.05,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
target 20260822.4568 12.64CV 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 22.4568 2461274.9568 12.52 10:12:18.92 +61:11:49.1
149.70340 46.81098 galactic UMa Second-epoch detections are separated by 1.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:18.92 +61:11:49.1 (user input) | T | P | (position from user input) J-Ks=0.317+/-0.033 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:12:18.92 +61:11:49.1: 13.81 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:12:18.92 +61:11:49.1: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 12 18.92 +61 11 49.1 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4568 12.52CV 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 22.4568 2461274.9568 12.54 10:08:15.86 +60:16:27.3
151.22988 46.89270 galactic UMa Second-epoch detections are separated by 2.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:08:15.86 +60:16:27.3 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.032 (G)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:08:15.86 +60:16:27.3: 13.77 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:08:15.86 +60:16:27.3: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 08 15.86 +60 16 27.3 12.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.54,0.05,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
target 20260822.4568 12.54CV 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 22.4568 2461274.9568 12.55 10:16:35.41 +62:03:01.6
148.25661 46.74292 galactic UMa Second-epoch detections are separated by 2.0" and 6.9 pix
The object was found in VSX 3" Gaia DR3 1052013520026012800
Type: ROT
# Max. Min./Amp. JD0 Period
12.970 G 12.990 G M
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:16:35.41 +62:03:01.6: 13.76 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:16:35.41 +62:03:01.6: 13.76 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 16 35.41 +62 03 01.6 12.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1052013520026012800,2461274.9568,12.55,0.05,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 1052013520026012800 20260822.4568 12.55CV 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 22.4568 2461274.9568 12.32 10:08:20.34 +59:49:47.7
151.77838 47.13282 galactic UMa Second-epoch detections are separated by 2.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:08:20.34 +59:49:47.7 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.032 (F)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:08:20.34 +59:49:47.7: 13.77 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-22_00-30-42_20.00sec_-14.90C_LIGHT_0276.fits at 10:08:20.34 +59:49:47.7: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4568* 10 08 20.34 +59 49 47.7 12.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.9568,12.32,0.05,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
target 20260822.4568 12.32CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.80575086 11.02.2026 07:20:06.874 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
First image: 2461082.80575086 11.02.2026 07:20:06.874 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
Last image: 2461274.95707081 22.08.2026 10:58:00.918 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_UMa-03-Q1b1x1_055851_TTUQ1b1x1_2579400_WLmt4Jj0/fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 3 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): 7552
Objects passed selection criteria: 7503
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: 4729.75
Average stars matched: 4513 (95.4173 %)
Memory usage VmPeak: 233764 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 06:03:02 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.80575086 11.02.2026 07:20:06.874 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
First image: 2461082.80575086 11.02.2026 07:20:06.874 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
Last image: 2461274.95707081 22.08.2026 10:58:00.918 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_UMa-03-Q1b1x1_055851_TTUQ1b1x1_2579400_WLmt4Jj0/fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 188
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.23
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: 15 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): 40221
Objects passed selection criteria: 40094
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 26302.5
Average stars matched: 25234.5 (95.9395 %)
Memory usage VmPeak: 262680 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 06:03:56 CDT 2026
Host name: tau
############################################################
**** FOUND 09:10:57.40 +63:32:53.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53539_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
The candidate 53539_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211 did not pass the final checks
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Considering the candidate 53853_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
The candidate 53853_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211 did not pass the final checks
**** FOUND 09:20:40.63 +57:37:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54055_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
The candidate 54055_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211 did not pass the final checks
Rejecting candidate due to large distance (29.8") between the two second-epoch detections
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Considering the candidate 13175_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 13175_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 16224_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 16224_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 30966_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 30966_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 13746_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 13746_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 08368_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 08368_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 15950_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 15950_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 15011_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 15011_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 10919_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 10919_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 11250_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 11250_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 33995_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 33995_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 21415_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 21415_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 20693_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 20693_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 08692_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 08692_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 13266_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 13266_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 16164_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 16164_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 39060_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 39060_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 51404_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
The candidate 51404_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211 did not pass the final checks
Rejecting candidate due to large distance (41.6") between the two second-epoch detections
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Considering the candidate 24264_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 24264_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 27621_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 27621_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 34615_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 34615_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 40357_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 40357_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 17023_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 17023_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 40075_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 40075_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 32308_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 32308_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 10132_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 10132_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 34483_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 34483_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 14973_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 14973_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 19386_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 19386_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 09310_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 09310_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 18149_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 18149_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 25530_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 25530_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 13198_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 13198_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 36041_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 36041_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 14718_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 14718_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 34427_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 34427_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 22885_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 22885_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 36069_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 36069_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 18301_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 18301_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 16112_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 16112_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 27612_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 27612_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 38943_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 38943_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 17834_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 17834_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 17494_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 17494_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 12134_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 12134_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 36871_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 36871_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 35857_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 35857_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 19087_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
The candidate 19087_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211 did not pass the final checks
Rejecting candidate due to large distance (43.0") between the two second-epoch detections
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Considering the candidate 21897_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 21897_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 38918_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 38918_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 17638_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 17638_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 36363_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 36363_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 32306_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 32306_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 14585_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 14585_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 09750_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 09750_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 42462_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 42462_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 32996_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 32996_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 38465_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 38465_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 36492_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 36492_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 29488_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 29488_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 16853_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 16853_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 33116_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 33116_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 33258_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 33258_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 08783_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 08783_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 12498_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 12498_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 39606_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 39606_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 24103_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 24103_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 15740_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 15740_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 08315_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 08315_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 14111_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 14111_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 22652_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 22652_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 17361_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 17361_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 08506_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 08506_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 34693_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 34693_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 34927_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 34927_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 20289_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 20289_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 11034_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
The candidate 11034_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211 did not pass the final checks
**** FOUND 10:36:17.29 +59:56:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12133_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 12133_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 21332_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 21332_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 36557_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 36557_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 10183_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 10183_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 08498_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 08498_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 19499_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 19499_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 15765_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 15765_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 21471_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 21471_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 14750_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 14750_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 16805_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 16805_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 25864_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 25864_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 10130_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 10130_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 09517_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 09517_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 34202_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 34202_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 16872_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 16872_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 33575_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 33575_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 07573_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 07573_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 08253_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 08253_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 19149_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 19149_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 12486_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 12486_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 13115_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 13115_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 32600_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 32600_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 24365_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 24365_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 17720_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 17720_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 14081_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 14081_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 36526_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 36526_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 10309_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 10309_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 20570_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 20570_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 16316_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 16316_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 11145_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 11145_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 38873_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 38873_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 35668_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 35668_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 30551_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 30551_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 22193_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 22193_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 10665_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 10665_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 11093_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 11093_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 20261_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 20261_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 18600_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 18600_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 22364_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 22364_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 11383_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 11383_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 09849_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 09849_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 41239_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 41239_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 09874_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 09874_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 18197_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 18197_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 16778_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 16778_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 15772_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 15772_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 16948_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 16948_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 12386_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 12386_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 12668_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 12668_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 16262_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 16262_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 04044_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 04044_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 06663_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 06663_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 18081_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 18081_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 09858_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 09858_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 31161_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 31161_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 39855_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 39855_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 27416_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
The candidate 27416_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211 did not pass the final checks
**** FOUND 09:22:10.37 +65:19:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18067_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 18067_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 15601_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 15601_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 24579_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 24579_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 03648_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 03648_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 15205_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 15205_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 33923_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 33923_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 20457_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 20457_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 17431_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 17431_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 12400_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 12400_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 11064_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 11064_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 09433_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 09433_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 13958_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 13958_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 20032_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 20032_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 05405_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 05405_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 05835_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 05835_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 04479_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 04479_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 24452_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 24452_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 11193_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 11193_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 15888_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 15888_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 07087_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 07087_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 16076_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 16076_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 15760_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 15760_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 11580_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 11580_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 17884_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 17884_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 17064_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
The candidate 17064_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211 did not pass the final checks
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Considering the candidate 11316_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 11316_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 15325_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 15325_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 08236_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 08236_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 11228_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 11228_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 14210_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 14210_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 31585_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 31585_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 12634_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 12634_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 08735_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 08735_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 14325_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 14325_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 15336_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 15336_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 12384_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 12384_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 05518_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 05518_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 13838_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 13838_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 12806_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 12806_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 35330_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 35330_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 19110_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 19110_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 17322_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 17322_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 13919_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 13919_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 20606_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 20606_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
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Considering the candidate 12168_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
Preparing report for the candidate 12168_fd_UMa-03-Q1b1x1_2026-08-22_05-58-00_20.00sec_-0.00C_LIGHTs_0211
make_report_in_HTML.sh Phase 2 (HTML assembly): 9s
make_report_in_HTML.sh TOTAL: 3562s
Prepared the HTML report for the field UMa-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:57:57.86 +57:18:25.6
09:52:08.82 +57:15:33.6
09:56:36.25 +57:30:28.6
10:07:05.17 +58:02:21.7
09:47:28.49 +57:33:32.3
09:55:58.76 +57:53:34.4
10:04:08.19 +58:18:37.8
09:55:49.10 +58:12:57.3
09:57:52.91 +58:24:03.5
10:00:30.51 +58:38:27.4
09:57:29.91 +58:33:56.7
10:12:56.61 +58:55:04.6
10:00:53.61 +58:41:07.5
10:01:33.08 +58:44:06.4
09:58:56.54 +58:40:26.8
10:08:56.14 +58:56:53.4
09:58:37.16 +58:44:06.8
09:52:00.81 +58:34:14.1
09:57:32.66 +58:51:43.9
09:57:08.65 +58:53:29.2
09:59:52.04 +58:58:53.3
10:07:54.95 +59:13:22.3
10:03:46.88 +59:09:42.3
10:08:24.15 +59:15:31.6
10:02:24.15 +59:08:11.8
09:58:36.71 +59:06:52.5
10:01:47.99 +59:11:07.4
09:59:39.78 +59:08:56.2
10:10:49.67 +59:25:25.9
10:01:48.91 +59:19:34.4
10:05:06.18 +59:27:47.4
10:15:56.25 +59:41:47.2
10:06:27.02 +59:31:55.2
09:59:57.05 +59:24:09.5
09:58:53.69 +59:23:23.5
09:57:59.53 +59:22:39.0
10:00:32.05 +59:26:27.5
10:14:31.42 +59:43:49.7
10:18:05.01 +59:48:06.0
10:03:14.12 +59:34:59.3
10:19:57.73 +60:01:01.0
09:57:35.03 +59:35:02.8
10:08:20.34 +59:49:47.7
10:08:15.86 +59:55:29.8
10:06:16.55 +59:51:03.8
10:14:37.24 +60:00:22.3
09:57:12.38 +59:40:13.4
10:07:46.74 +59:54:28.0
10:04:53.11 +59:53:18.4
10:05:21.03 +59:54:08.2
10:21:20.89 +60:12:30.3
10:18:02.30 +60:14:24.3
10:09:56.10 +60:07:24.8
10:04:12.93 +60:00:34.1
10:02:06.48 +60:00:16.5
10:14:35.88 +60:21:09.9
10:17:31.60 +60:25:32.1
10:08:15.86 +60:16:27.3
10:21:28.39 +60:30:27.4
10:06:16.40 +60:17:19.1
10:10:28.32 +60:22:32.5
10:15:15.66 +60:29:19.5
10:09:14.07 +60:24:51.6
10:18:02.98 +60:36:41.2
10:09:43.41 +60:30:07.7
10:17:43.89 +60:38:42.3
10:14:01.02 +60:38:09.5
10:12:57.86 +60:37:56.3
10:16:57.68 +60:44:25.6
10:23:57.27 +60:51:54.5
10:08:00.96 +60:37:32.6
10:25:21.16 +60:56:52.2
10:11:59.03 +60:47:46.8
10:11:49.64 +60:47:49.0
10:21:15.15 +60:56:22.7
10:06:44.77 +60:42:28.8
10:23:42.01 +61:00:02.0
10:18:28.95 +60:56:51.6
10:18:31.41 +60:59:24.5
10:21:38.43 +61:02:07.5
10:16:18.66 +60:58:39.7
10:26:23.35 +61:07:26.3
10:26:55.65 +61:08:00.0
10:10:31.95 +60:55:20.5
10:27:00.03 +61:15:52.5
10:16:34.37 +61:08:33.6
10:15:54.42 +61:08:36.0
10:08:25.45 +61:01:15.9
10:12:38.50 +61:07:06.7
10:17:14.42 +61:11:51.6
10:12:18.92 +61:11:49.1
10:10:17.45 +61:10:40.8
10:25:52.64 +61:24:47.5
10:25:03.56 +61:25:13.7
10:15:48.11 +61:20:12.1
10:16:15.69 +61:21:27.8
10:19:44.11 +61:26:10.0
10:11:35.54 +61:19:40.9
10:16:48.91 +61:27:26.6
10:20:55.01 +61:30:55.6
10:09:40.01 +61:21:23.2
10:26:43.74 +61:36:14.2
10:17:40.97 +61:31:06.9
10:19:49.79 +61:37:46.1
10:16:33.89 +61:41:53.2
10:17:29.85 +61:43:41.3
10:18:58.47 +61:47:58.7
10:25:54.31 +61:54:44.0
10:18:44.24 +61:57:16.8
10:27:21.73 +62:06:51.9
10:16:12.41 +61:58:36.4
10:18:46.00 +62:03:32.2
10:20:35.71 +62:06:21.9
10:16:35.41 +62:03:01.6
10:25:58.84 +62:11:55.0
10:27:08.49 +62:22:09.7
10:16:27.10 +62:14:32.0
10:29:20.30 +62:23:55.3
10:22:36.19 +62:25:55.7
10:47:07.03 +62:39:22.2
10:29:23.58 +62:36:56.6
10:25:26.20 +62:38:46.4
10:30:00.03 +62:44:35.8
10:34:54.53 +63:04:05.2
10:25:29.57 +63:01:49.8
10:27:31.05 +63:04:43.3
10:35:25.53 +63:09:04.7
10:30:11.78 +63:08:48.5
09:35:34.28 +66:16:46.3
09:08:56.09 +65:12:52.3
09:15:03.83 +64:59:59.6
09:29:27.57 +65:31:50.6
10:52:45.69 +64:57:24.9
10:41:02.20 +63:31:05.1
10:29:50.96 +63:22:58.8
10:34:12.40 +63:20:41.7
10:25:43.74 +63:09:53.5
09:31:31.05 +65:17:30.6
09:18:53.59 +64:52:04.7
09:18:25.57 +64:42:41.2
09:09:19.97 +64:15:25.3
09:13:51.94 +64:25:21.8
09:21:24.76 +64:41:50.3
09:15:38.54 +64:21:11.7
09:14:54.25 +64:11:42.9
09:22:15.59 +64:30:48.0
09:21:17.46 +64:22:14.5
09:21:44.85 +64:24:23.1
09:19:16.70 +64:13:48.8
09:14:01.47 +62:51:05.9
09:10:22.44 +62:33:04.4
09:20:02.31 +64:09:13.5
09:21:32.11 +64:07:07.1
09:13:47.07 +63:41:47.8
09:13:21.50 +63:36:01.9
09:10:23.61 +63:26:52.2
09:21:57.62 +63:49:12.1
09:12:25.54 +63:26:37.1
09:20:10.04 +63:43:52.2
09:13:33.47 +63:26:22.6
09:15:47.87 +63:31:49.6
09:21:12.13 +63:39:58.8
09:13:43.22 +62:51:10.3
09:14:34.67 +62:46:18.7
09:11:46.71 +62:38:39.3
09:17:12.51 +62:53:36.1
09:15:44.90 +62:46:56.5
09:15:49.88 +62:36:39.5
09:10:52.85 +62:18:17.8
09:12:36.44 +62:20:01.5
09:16:12.60 +62:25:51.4
10:37:03.90 +63:58:35.7
10:31:02.44 +63:36:47.0
########### Completed UMa-03-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 ####
10:09:56.10 +60:07:24.8
10:26:23.35 +61:07:26.3
10:29:50.96 +63:22:58.8
10:14:35.88 +60:21:09.9
10:00:53.61 +58:41:07.5
10:18:28.95 +60:56:51.6
10:12:57.86 +60:37:56.3
10:05:06.18 +59:27:47.4
10:00:32.05 +59:26:27.5
09:22:15.59 +64:30:48.0
10:16:27.10 +62:14:32.0
10:25:58.84 +62:11:55.0
10:08:56.14 +58:56:53.4
10:02:06.48 +60:00:16.5
10:16:18.66 +60:58:39.7
09:15:44.90 +62:46:56.5
10:25:29.57 +63:01:49.8
09:29:27.57 +65:31:50.6
09:14:01.47 +62:51:05.9
09:16:12.60 +62:25:51.4
10:17:14.42 +61:11:51.6
09:12:36.44 +62:20:01.5
09:18:53.59 +64:52:04.7
10:01:47.99 +59:11:07.4
09:19:16.70 +64:13:48.8
10:14:01.02 +60:38:09.5
10:18:58.47 +61:47:58.7
09:57:32.66 +58:51:43.9
10:09:40.01 +61:21:23.2
09:35:34.28 +66:16:46.3
10:04:12.93 +60:00:34.1
09:10:23.61 +63:26:52.2
10:09:43.41 +60:30:07.7
09:21:44.85 +64:24:23.1
10:30:00.03 +62:44:35.8
09:21:57.62 +63:49:12.1
10:17:40.97 +61:31:06.9
10:21:38.43 +61:02:07.5
09:15:03.83 +64:59:59.6
09:17:12.51 +62:53:36.1
10:19:44.11 +61:26:10.0
10:25:03.56 +61:25:13.7
09:57:35.03 +59:35:02.8
09:21:12.13 +63:39:58.8
09:13:21.50 +63:36:01.9
10:22:36.19 +62:25:55.7
09:11:46.71 +62:38:39.3
10:15:48.11 +61:20:12.1
09:12:25.54 +63:26:37.1
09:31:31.05 +65:17:30.6
10:18:02.98 +60:36:41.2
10:07:54.95 +59:13:22.3
10:31:02.44 +63:36:47.0
09:09:19.97 +64:15:25.3
09:13:43.22 +62:51:10.3
09:20:10.04 +63:43:52.2
10:52:45.69 +64:57:24.9
10:15:54.42 +61:08:36.0
09:13:51.94 +64:25:21.8
09:21:24.76 +64:41:50.3
09:52:00.81 +58:34:14.1
10:07:46.74 +59:54:28.0
09:15:49.88 +62:36:39.5
10:34:54.53 +63:04:05.2
10:11:59.03 +60:47:46.8
10:12:56.61 +58:55:04.6
10:10:28.32 +60:22:32.5
10:25:26.20 +62:38:46.4
10:10:17.45 +61:10:40.8
09:58:56.54 +58:40:26.8
09:10:22.44 +62:33:04.4
09:20:02.31 +64:09:13.5
10:16:12.41 +61:58:36.4
10:19:57.73 +60:01:01.0
10:27:08.49 +62:22:09.7
09:15:47.87 +63:31:49.6
09:59:39.78 +59:08:56.2
10:01:33.08 +58:44:06.4
10:25:54.31 +61:54:44.0
10:21:15.15 +60:56:22.7
10:29:20.30 +62:23:55.3
10:17:43.89 +60:38:42.3
10:16:34.37 +61:08:33.6
09:08:56.09 +65:12:52.3
09:58:36.71 +59:06:52.5
09:59:52.04 +58:58:53.3
09:21:17.46 +64:22:14.5
10:08:25.45 +61:01:15.9
09:15:38.54 +64:21:11.7
09:57:52.91 +58:24:03.5
09:57:29.91 +58:33:56.7
10:17:29.85 +61:43:41.3
09:57:12.38 +59:40:13.4
10:18:02.30 +60:14:24.3
09:18:25.57 +64:42:41.2
10:27:31.05 +63:04:43.3
10:16:15.69 +61:21:27.8
10:06:16.40 +60:17:19.1
09:13:33.47 +63:26:22.6
10:10:49.67 +59:25:25.9
10:20:35.71 +62:06:21.9
10:10:31.95 +60:55:20.5
09:59:57.05 +59:24:09.5
09:14:34.67 +62:46:18.7
09:13:47.07 +63:41:47.8
10:41:02.20 +63:31:05.1
10:47:07.03 +62:39:22.2
10:01:48.91 +59:19:34.4
10:06:27.02 +59:31:55.2
10:27:21.73 +62:06:51.9
10:19:49.79 +61:37:46.1
10:29:23.58 +62:36:56.6
10:18:05.01 +59:48:06.0
10:03:46.88 +59:09:42.3
10:37:03.90 +63:58:35.7
10:02:24.15 +59:08:11.8
10:26:43.74 +61:36:14.2
10:27:00.03 +61:15:52.5
10:06:44.77 +60:42:28.8
10:12:38.50 +61:07:06.7
10:06:16.55 +59:51:03.8
10:05:21.03 +59:54:08.2
10:26:55.65 +61:08:00.0
09:52:08.82 +57:15:33.6
10:04:08.19 +58:18:37.8
10:20:55.01 +61:30:55.6
10:08:24.15 +59:15:31.6
10:34:12.40 +63:20:41.7
09:10:52.85 +62:18:17.8
10:16:48.91 +61:27:26.6
10:25:21.16 +60:56:52.2
10:30:11.78 +63:08:48.5
09:57:57.86 +57:18:25.6
10:16:57.68 +60:44:25.6
09:14:54.25 +64:11:42.9
10:18:46.00 +62:03:32.2
10:25:52.64 +61:24:47.5
10:14:37.24 +60:00:22.3
10:15:56.25 +59:41:47.2
09:57:08.65 +58:53:29.2
10:21:28.39 +60:30:27.4
10:18:44.24 +61:57:16.8
10:07:05.17 +58:02:21.7
09:55:58.76 +57:53:34.4
09:56:36.25 +57:30:28.6
10:35:25.53 +63:09:04.7
09:58:53.69 +59:23:23.5
10:23:42.01 +61:00:02.0
09:55:49.10 +58:12:57.3
10:18:31.41 +60:59:24.5
10:11:49.64 +60:47:49.0
10:03:14.12 +59:34:59.3
10:11:35.54 +61:19:40.9
10:14:31.42 +59:43:49.7
10:23:57.27 +60:51:54.5
10:00:30.51 +58:38:27.4
09:57:59.53 +59:22:39.0
10:15:15.66 +60:29:19.5
10:25:43.74 +63:09:53.5
10:04:53.11 +59:53:18.4
09:58:37.16 +58:44:06.8
10:09:14.07 +60:24:51.6
10:08:00.96 +60:37:32.6
10:08:15.86 +59:55:29.8
09:47:28.49 +57:33:32.3
10:17:31.60 +60:25:32.1
10:21:20.89 +60:12:30.3
09:21:32.11 +64:07:07.1
10:16:33.89 +61:41:53.2
10:12:18.92 +61:11:49.1
10:08:15.86 +60:16:27.3
10:16:35.41 +62:03:01.6
10:08:20.34 +59:49:47.7
###################################################################################
10:09:56.10 +60:07:24.8 -- not an asteroid (will add it to exclusion list)
10:26:23.35 +61:07:26.3 -- not an asteroid (will add it to exclusion list)
10:29:50.96 +63:22:58.8 -- not an asteroid (will add it to exclusion list)
10:14:35.88 +60:21:09.9 -- not an asteroid (will add it to exclusion list)
10:00:53.61 +58:41:07.5 -- not an asteroid (will add it to exclusion list)
10:18:28.95 +60:56:51.6 -- not an asteroid (will add it to exclusion list)
10:12:57.86 +60:37:56.3 -- not an asteroid (will add it to exclusion list)
10:05:06.18 +59:27:47.4 -- not an asteroid (will add it to exclusion list)
10:00:32.05 +59:26:27.5 -- not an asteroid (will add it to exclusion list)
09:22:15.59 +64:30:48.0 -- not an asteroid (will add it to exclusion list)
10:16:27.10 +62:14:32.0 -- not an asteroid (will add it to exclusion list)
10:25:58.84 +62:11:55.0 -- not an asteroid (will add it to exclusion list)
10:08:56.14 +58:56:53.4 -- not an asteroid (will add it to exclusion list)
10:02:06.48 +60:00:16.5 -- not an asteroid (will add it to exclusion list)
10:16:18.66 +60:58:39.7 -- not an asteroid (will add it to exclusion list)
09:15:44.90 +62:46:56.5 -- not an asteroid (will add it to exclusion list)
10:25:29.57 +63:01:49.8 -- not an asteroid (will add it to exclusion list)
09:29:27.57 +65:31:50.6 -- not an asteroid (will add it to exclusion list)
09:14:01.47 +62:51:05.9 -- not an asteroid (will add it to exclusion list)
09:16:12.60 +62:25:51.4 -- not an asteroid (will add it to exclusion list)
10:17:14.42 +61:11:51.6 -- not an asteroid (will add it to exclusion list)
09:12:36.44 +62:20:01.5 -- not an asteroid (will add it to exclusion list)
09:18:53.59 +64:52:04.7 -- not an asteroid (will add it to exclusion list)
10:01:47.99 +59:11:07.4 -- not an asteroid (will add it to exclusion list)
09:19:16.70 +64:13:48.8 -- not an asteroid (will add it to exclusion list)
10:14:01.02 +60:38:09.5 -- not an asteroid (will add it to exclusion list)
10:18:58.47 +61:47:58.7 -- not an asteroid (will add it to exclusion list)
09:57:32.66 +58:51:43.9 -- not an asteroid (will add it to exclusion list)
10:09:40.01 +61:21:23.2 -- not an asteroid (will add it to exclusion list)
09:35:34.28 +66:16:46.3 -- not an asteroid (will add it to exclusion list)
10:04:12.93 +60:00:34.1 -- not an asteroid (will add it to exclusion list)
09:10:23.61 +63:26:52.2 -- not an asteroid (will add it to exclusion list)
10:09:43.41 +60:30:07.7 -- not an asteroid (will add it to exclusion list)
09:21:44.85 +64:24:23.1 -- not an asteroid (will add it to exclusion list)
10:30:00.03 +62:44:35.8 -- not an asteroid (will add it to exclusion list)
09:21:57.62 +63:49:12.1 -- not an asteroid (will add it to exclusion list)
10:17:40.97 +61:31:06.9 -- not an asteroid (will add it to exclusion list)
10:21:38.43 +61:02:07.5 -- not an asteroid (will add it to exclusion list)
09:15:03.83 +64:59:59.6 -- not an asteroid (will add it to exclusion list)
09:17:12.51 +62:53:36.1 -- not an asteroid (will add it to exclusion list)
10:19:44.11 +61:26:10.0 -- not an asteroid (will add it to exclusion list)
10:25:03.56 +61:25:13.7 -- not an asteroid (will add it to exclusion list)
09:57:35.03 +59:35:02.8 -- not an asteroid (will add it to exclusion list)
09:21:12.13 +63:39:58.8 -- not an asteroid (will add it to exclusion list)
09:13:21.50 +63:36:01.9 -- not an asteroid (will add it to exclusion list)
10:22:36.19 +62:25:55.7 -- not an asteroid (will add it to exclusion list)
09:11:46.71 +62:38:39.3 -- not an asteroid (will add it to exclusion list)
10:15:48.11 +61:20:12.1 -- not an asteroid (will add it to exclusion list)
09:12:25.54 +63:26:37.1 -- not an asteroid (will add it to exclusion list)
09:31:31.05 +65:17:30.6 -- not an asteroid (will add it to exclusion list)
10:18:02.98 +60:36:41.2 -- not an asteroid (will add it to exclusion list)
10:07:54.95 +59:13:22.3 -- not an asteroid (will add it to exclusion list)
10:31:02.44 +63:36:47.0 -- not an asteroid (will add it to exclusion list)
09:09:19.97 +64:15:25.3 -- not an asteroid (will add it to exclusion list)
09:13:43.22 +62:51:10.3 -- not an asteroid (will add it to exclusion list)
09:20:10.04 +63:43:52.2 -- not an asteroid (will add it to exclusion list)
10:52:45.69 +64:57:24.9 -- not an asteroid (will add it to exclusion list)
10:15:54.42 +61:08:36.0 -- not an asteroid (will add it to exclusion list)
09:13:51.94 +64:25:21.8 -- not an asteroid (will add it to exclusion list)
09:21:24.76 +64:41:50.3 -- not an asteroid (will add it to exclusion list)
09:52:00.81 +58:34:14.1 -- not an asteroid (will add it to exclusion list)
10:07:46.74 +59:54:28.0 -- not an asteroid (will add it to exclusion list)
09:15:49.88 +62:36:39.5 -- not an asteroid (will add it to exclusion list)
10:34:54.53 +63:04:05.2 -- not an asteroid (will add it to exclusion list)
10:11:59.03 +60:47:46.8 -- not an asteroid (will add it to exclusion list)
10:12:56.61 +58:55:04.6 -- not an asteroid (will add it to exclusion list)
10:10:28.32 +60:22:32.5 -- not an asteroid (will add it to exclusion list)
10:25:26.20 +62:38:46.4 -- not an asteroid (will add it to exclusion list)
10:10:17.45 +61:10:40.8 -- not an asteroid (will add it to exclusion list)
09:58:56.54 +58:40:26.8 -- not an asteroid (will add it to exclusion list)
09:10:22.44 +62:33:04.4 -- not an asteroid (will add it to exclusion list)
09:20:02.31 +64:09:13.5 -- not an asteroid (will add it to exclusion list)
10:16:12.41 +61:58:36.4 -- not an asteroid (will add it to exclusion list)
10:19:57.73 +60:01:01.0 -- not an asteroid (will add it to exclusion list)
10:27:08.49 +62:22:09.7 -- not an asteroid (will add it to exclusion list)
09:15:47.87 +63:31:49.6 -- not an asteroid (will add it to exclusion list)
09:59:39.78 +59:08:56.2 -- not an asteroid (will add it to exclusion list)
10:01:33.08 +58:44:06.4 -- not an asteroid (will add it to exclusion list)
10:25:54.31 +61:54:44.0 -- not an asteroid (will add it to exclusion list)
10:21:15.15 +60:56:22.7 -- not an asteroid (will add it to exclusion list)
10:29:20.30 +62:23:55.3 -- not an asteroid (will add it to exclusion list)
10:17:43.89 +60:38:42.3 -- not an asteroid (will add it to exclusion list)
10:16:34.37 +61:08:33.6 -- not an asteroid (will add it to exclusion list)
09:08:56.09 +65:12:52.3 -- not an asteroid (will add it to exclusion list)
09:58:36.71 +59:06:52.5 -- not an asteroid (will add it to exclusion list)
09:59:52.04 +58:58:53.3 -- not an asteroid (will add it to exclusion list)
09:21:17.46 +64:22:14.5 -- not an asteroid (will add it to exclusion list)
10:08:25.45 +61:01:15.9 -- not an asteroid (will add it to exclusion list)
09:15:38.54 +64:21:11.7 -- not an asteroid (will add it to exclusion list)
09:57:52.91 +58:24:03.5 -- not an asteroid (will add it to exclusion list)
09:57:29.91 +58:33:56.7 -- not an asteroid (will add it to exclusion list)
10:17:29.85 +61:43:41.3 -- not an asteroid (will add it to exclusion list)
09:57:12.38 +59:40:13.4 -- not an asteroid (will add it to exclusion list)
10:18:02.30 +60:14:24.3 -- not an asteroid (will add it to exclusion list)
09:18:25.57 +64:42:41.2 -- not an asteroid (will add it to exclusion list)
10:27:31.05 +63:04:43.3 -- not an asteroid (will add it to exclusion list)
10:16:15.69 +61:21:27.8 -- not an asteroid (will add it to exclusion list)
10:06:16.40 +60:17:19.1 -- not an asteroid (will add it to exclusion list)
09:13:33.47 +63:26:22.6 -- not an asteroid (will add it to exclusion list)
10:10:49.67 +59:25:25.9 -- not an asteroid (will add it to exclusion list)
10:20:35.71 +62:06:21.9 -- not an asteroid (will add it to exclusion list)
10:10:31.95 +60:55:20.5 -- not an asteroid (will add it to exclusion list)
09:59:57.05 +59:24:09.5 -- not an asteroid (will add it to exclusion list)
09:14:34.67 +62:46:18.7 -- not an asteroid (will add it to exclusion list)
09:13:47.07 +63:41:47.8 -- not an asteroid (will add it to exclusion list)
10:41:02.20 +63:31:05.1 -- not an asteroid (will add it to exclusion list)
10:47:07.03 +62:39:22.2 -- not an asteroid (will add it to exclusion list)
10:01:48.91 +59:19:34.4 -- not an asteroid (will add it to exclusion list)
10:06:27.02 +59:31:55.2 -- not an asteroid (will add it to exclusion list)
10:27:21.73 +62:06:51.9 -- not an asteroid (will add it to exclusion list)
10:19:49.79 +61:37:46.1 -- not an asteroid (will add it to exclusion list)
10:29:23.58 +62:36:56.6 -- not an asteroid (will add it to exclusion list)
10:18:05.01 +59:48:06.0 -- not an asteroid (will add it to exclusion list)
10:03:46.88 +59:09:42.3 -- not an asteroid (will add it to exclusion list)
10:37:03.90 +63:58:35.7 -- not an asteroid (will add it to exclusion list)
10:02:24.15 +59:08:11.8 -- not an asteroid (will add it to exclusion list)
10:26:43.74 +61:36:14.2 -- not an asteroid (will add it to exclusion list)
10:27:00.03 +61:15:52.5 -- not an asteroid (will add it to exclusion list)
10:06:44.77 +60:42:28.8 -- not an asteroid (will add it to exclusion list)
10:12:38.50 +61:07:06.7 -- not an asteroid (will add it to exclusion list)
10:06:16.55 +59:51:03.8 -- not an asteroid (will add it to exclusion list)
10:05:21.03 +59:54:08.2 -- not an asteroid (will add it to exclusion list)
10:26:55.65 +61:08:00.0 -- not an asteroid (will add it to exclusion list)
09:52:08.82 +57:15:33.6 -- not an asteroid (will add it to exclusion list)
10:04:08.19 +58:18:37.8 -- not an asteroid (will add it to exclusion list)
10:20:55.01 +61:30:55.6 -- not an asteroid (will add it to exclusion list)
10:08:24.15 +59:15:31.6 -- not an asteroid (will add it to exclusion list)
10:34:12.40 +63:20:41.7 -- not an asteroid (will add it to exclusion list)
09:10:52.85 +62:18:17.8 -- not an asteroid (will add it to exclusion list)
10:16:48.91 +61:27:26.6 -- not an asteroid (will add it to exclusion list)
10:25:21.16 +60:56:52.2 -- not an asteroid (will add it to exclusion list)
10:30:11.78 +63:08:48.5 -- not an asteroid (will add it to exclusion list)
09:57:57.86 +57:18:25.6 -- not an asteroid (will add it to exclusion list)
10:16:57.68 +60:44:25.6 -- not an asteroid (will add it to exclusion list)
09:14:54.25 +64:11:42.9 -- not an asteroid (will add it to exclusion list)
10:18:46.00 +62:03:32.2 -- not an asteroid (will add it to exclusion list)
10:25:52.64 +61:24:47.5 -- not an asteroid (will add it to exclusion list)
10:14:37.24 +60:00:22.3 -- not an asteroid (will add it to exclusion list)
10:15:56.25 +59:41:47.2 -- not an asteroid (will add it to exclusion list)
09:57:08.65 +58:53:29.2 -- not an asteroid (will add it to exclusion list)
10:21:28.39 +60:30:27.4 -- not an asteroid (will add it to exclusion list)
10:18:44.24 +61:57:16.8 -- not an asteroid (will add it to exclusion list)
10:07:05.17 +58:02:21.7 -- not an asteroid (will add it to exclusion list)
09:55:58.76 +57:53:34.4 -- not an asteroid (will add it to exclusion list)
09:56:36.25 +57:30:28.6 -- not an asteroid (will add it to exclusion list)
10:35:25.53 +63:09:04.7 -- not an asteroid (will add it to exclusion list)
09:58:53.69 +59:23:23.5 -- not an asteroid (will add it to exclusion list)
10:23:42.01 +61:00:02.0 -- not an asteroid (will add it to exclusion list)
09:55:49.10 +58:12:57.3 -- not an asteroid (will add it to exclusion list)
10:18:31.41 +60:59:24.5 -- not an asteroid (will add it to exclusion list)
10:11:49.64 +60:47:49.0 -- not an asteroid (will add it to exclusion list)
10:03:14.12 +59:34:59.3 -- not an asteroid (will add it to exclusion list)
10:11:35.54 +61:19:40.9 -- not an asteroid (will add it to exclusion list)
10:14:31.42 +59:43:49.7 -- not an asteroid (will add it to exclusion list)
10:23:57.27 +60:51:54.5 -- not an asteroid (will add it to exclusion list)
10:00:30.51 +58:38:27.4 -- not an asteroid (will add it to exclusion list)
09:57:59.53 +59:22:39.0 -- not an asteroid (will add it to exclusion list)
10:15:15.66 +60:29:19.5 -- not an asteroid (will add it to exclusion list)
10:25:43.74 +63:09:53.5 -- not an asteroid (will add it to exclusion list)
10:04:53.11 +59:53:18.4 -- not an asteroid (will add it to exclusion list)
09:58:37.16 +58:44:06.8 -- not an asteroid (will add it to exclusion list)
10:09:14.07 +60:24:51.6 -- not an asteroid (will add it to exclusion list)
10:08:00.96 +60:37:32.6 -- not an asteroid (will add it to exclusion list)
10:08:15.86 +59:55:29.8 -- not an asteroid (will add it to exclusion list)
09:47:28.49 +57:33:32.3 -- not an asteroid (will add it to exclusion list)
10:17:31.60 +60:25:32.1 -- not an asteroid (will add it to exclusion list)
10:21:20.89 +60:12:30.3 -- not an asteroid (will add it to exclusion list)
09:21:32.11 +64:07:07.1 -- not an asteroid (will add it to exclusion list)
10:16:33.89 +61:41:53.2 -- not an asteroid (will add it to exclusion list)
10:12:18.92 +61:11:49.1 -- not an asteroid (will add it to exclusion list)
10:08:15.86 +60:16:27.3 -- not an asteroid (will add it to exclusion list)
10:16:35.41 +62:03:01.6 -- not an asteroid (will add it to exclusion list)
10:08:20.34 +59:49:47.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
09:08:56.09 +65:12:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:09:19.97 +64:15:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:22.44 +62:33:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:23.61 +63:26:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:52.85 +62:18:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:46.71 +62:38:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:25.54 +63:26:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:36.44 +62:20:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:13:21.50 +63:36:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:13:33.47 +63:26:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:13:43.22 +62:51:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:13:47.07 +63:41:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:13:51.94 +64:25:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:14:01.47 +62:51:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:14:34.67 +62:46:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:14:54.25 +64:11:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:15:03.83 +64:59:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:15:38.54 +64:21:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:15:44.90 +62:46:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:15:47.87 +63:31:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:15:49.88 +62:36:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:16:12.60 +62:25:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:17:12.51 +62:53:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:18:25.57 +64:42:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:18:53.59 +64:52:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:19:16.70 +64:13:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:20:02.31 +64:09:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:20:10.04 +63:43:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:12.13 +63:39:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:17.46 +64:22:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:24.76 +64:41:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:32.11 +64:07:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:44.85 +64:24:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:21:57.62 +63:49:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:15.59 +64:30:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:29:27.57 +65:31:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:31:31.05 +65:17:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:35:34.28 +66:16:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:47:28.49 +57:33:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:52:00.81 +58:34:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:52:08.82 +57:15:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:55:49.10 +58:12:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:55:58.76 +57:53:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:56:36.25 +57:30:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:57:08.65 +58:53:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:57:12.38 +59:40:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
09:57:29.91 +58:33:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
09:57:32.66 +58:51:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
09:57:35.03 +59:35:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:57:52.91 +58:24:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:57:57.86 +57:18:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
09:57:59.53 +59:22:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
09:58:36.71 +59:06:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:58:37.16 +58:44:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:58:53.69 +59:23:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:58:56.54 +58:40:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:59:39.78 +59:08:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:59:52.04 +58:58:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:59:57.05 +59:24:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:00:30.51 +58:38:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:00:32.05 +59:26:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:00:53.61 +58:41:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:01:33.08 +58:44:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:01:47.99 +59:11:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:01:48.91 +59:19:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:02:06.48 +60:00:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:02:24.15 +59:08:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:03:14.12 +59:34:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:03:46.88 +59:09:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:04:08.19 +58:18:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:04:12.93 +60:00:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:04:53.11 +59:53:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:05:06.18 +59:27:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:05:21.03 +59:54:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:06:16.40 +60:17:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:06:16.55 +59:51:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:06:27.02 +59:31:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:06:44.77 +60:42:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:05.17 +58:02:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:46.74 +59:54:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:07:54.95 +59:13:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:00.96 +60:37:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:15.86 +59:55:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:15.86 +60:16:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:20.34 +59:49:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:24.15 +59:15:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:25.45 +61:01:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:08:56.14 +58:56:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:14.07 +60:24:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:40.01 +61:21:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:43.41 +60:30:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:09:56.10 +60:07:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:17.45 +61:10:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:28.32 +60:22:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:31.95 +60:55:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:10:49.67 +59:25:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:35.54 +61:19:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:49.64 +60:47:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:11:59.03 +60:47:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:18.92 +61:11:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:38.50 +61:07:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:56.61 +58:55:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:12:57.86 +60:37:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:14:01.02 +60:38:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:14:31.42 +59:43:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:14:35.88 +60:21:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:14:37.24 +60:00:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:15:15.66 +60:29:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:15:48.11 +61:20:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:15:54.42 +61:08:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:15:56.25 +59:41:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:16:12.41 +61:58:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:16:15.69 +61:21:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:16:18.66 +60:58:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:16:27.10 +62:14:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:16:33.89 +61:41:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:16:34.37 +61:08:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:16:35.41 +62:03:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:16:48.91 +61:27:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:16:57.68 +60:44:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:17:14.42 +61:11:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:17:29.85 +61:43:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:17:31.60 +60:25:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:17:40.97 +61:31:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:17:43.89 +60:38:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:18:02.30 +60:14:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:18:02.98 +60:36:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:18:05.01 +59:48:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:18:28.95 +60:56:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:18:31.41 +60:59:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:18:44.24 +61:57:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:18:46.00 +62:03:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:18:58.47 +61:47:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:19:44.11 +61:26:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:19:49.79 +61:37:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:19:57.73 +60:01:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:20:35.71 +62:06:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:20:55.01 +61:30:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:21:15.15 +60:56:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:21:20.89 +60:12:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:21:28.39 +60:30:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:21:38.43 +61:02:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:22:36.19 +62:25:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:23:42.01 +61:00:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:23:57.27 +60:51:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:25:03.56 +61:25:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:25:21.16 +60:56:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:25:26.20 +62:38:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
10:25:29.57 +63:01:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:25:43.74 +63:09:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:25:52.64 +61:24:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:25:54.31 +61:54:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:25:58.84 +62:11:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:26:23.35 +61:07:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:26:43.74 +61:36:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:26:55.65 +61:08:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:27:00.03 +61:15:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:27:08.49 +62:22:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:27:21.73 +62:06:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
10:27:31.05 +63:04:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:29:20.30 +62:23:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
10:29:23.58 +62:36:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
10:29:50.96 +63:22:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:30:00.03 +62:44:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
10:30:11.78 +63:08:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
10:31:02.44 +63:36:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
10:34:12.40 +63:20:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:34:54.53 +63:04:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:35:25.53 +63:09:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:37:03.90 +63:58:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
10:41:02.20 +63:31:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
10:47:07.03 +62:39:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
10:52:45.69 +64:57:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
09:08:56.09 +65:12:52.3 -- not a known variable star
09:09:19.97 +64:15:25.3 -- not a known variable star
09:10:22.44 +62:33:04.4 -- not a known variable star
09:10:23.61 +63:26:52.2 -- not a known variable star
09:10:52.85 +62:18:17.8 -- not a known variable star
09:11:46.71 +62:38:39.3 -- not a known variable star
09:12:25.54 +63:26:37.1 -- not a known variable star
09:12:36.44 +62:20:01.5 -- not a known variable star
09:13:21.50 +63:36:01.9 -- a known variable star
09:13:33.47 +63:26:22.6 -- not a known variable star
09:13:43.22 +62:51:10.3 -- not a known variable star
09:13:47.07 +63:41:47.8 -- not a known variable star
09:13:51.94 +64:25:21.8 -- not a known variable star
09:14:01.47 +62:51:05.9 -- not a known variable star
09:14:34.67 +62:46:18.7 -- a known variable star
09:14:54.25 +64:11:42.9 -- not a known variable star
09:15:03.83 +64:59:59.6 -- not a known variable star
09:15:38.54 +64:21:11.7 -- not a known variable star
09:15:44.90 +62:46:56.5 -- not a known variable star
09:15:47.87 +63:31:49.6 -- not a known variable star
09:15:49.88 +62:36:39.5 -- not a known variable star
09:16:12.60 +62:25:51.4 -- not a known variable star
09:17:12.51 +62:53:36.1 -- not a known variable star
09:18:25.57 +64:42:41.2 -- not a known variable star
09:18:53.59 +64:52:04.7 -- not a known variable star
09:19:16.70 +64:13:48.8 -- not a known variable star
09:20:02.31 +64:09:13.5 -- not a known variable star
09:20:10.04 +63:43:52.2 -- not a known variable star
09:21:12.13 +63:39:58.8 -- a known variable star
09:21:17.46 +64:22:14.5 -- not a known variable star
09:21:24.76 +64:41:50.3 -- not a known variable star
09:21:32.11 +64:07:07.1 -- not a known variable star
09:21:44.85 +64:24:23.1 -- not a known variable star
09:21:57.62 +63:49:12.1 -- not a known variable star
09:22:15.59 +64:30:48.0 -- not a known variable star
09:29:27.57 +65:31:50.6 -- not a known variable star
09:31:31.05 +65:17:30.6 -- not a known variable star
09:35:34.28 +66:16:46.3 -- not a known variable star
09:47:28.49 +57:33:32.3 -- a known variable star
09:52:00.81 +58:34:14.1 -- a known variable star
09:52:08.82 +57:15:33.6 -- not a known variable star
09:55:49.10 +58:12:57.3 -- not a known variable star
09:55:58.76 +57:53:34.4 -- not a known variable star
09:56:36.25 +57:30:28.6 -- not a known variable star
09:57:08.65 +58:53:29.2 -- not a known variable star
09:57:12.38 +59:40:13.4 -- a known variable star
09:57:29.91 +58:33:56.7 -- a known variable star
09:57:32.66 +58:51:43.9 -- not a known variable star
09:57:35.03 +59:35:02.8 -- not a known variable star
09:57:52.91 +58:24:03.5 -- not a known variable star
09:57:57.86 +57:18:25.6 -- not a known variable star
09:57:59.53 +59:22:39.0 -- a known variable star
09:58:36.71 +59:06:52.5 -- not a known variable star
09:58:37.16 +58:44:06.8 -- not a known variable star
09:58:53.69 +59:23:23.5 -- not a known variable star
09:58:56.54 +58:40:26.8 -- not a known variable star
09:59:39.78 +59:08:56.2 -- not a known variable star
09:59:52.04 +58:58:53.3 -- not a known variable star
09:59:57.05 +59:24:09.5 -- not a known variable star
10:00:30.51 +58:38:27.4 -- not a known variable star
10:00:32.05 +59:26:27.5 -- not a known variable star
10:00:53.61 +58:41:07.5 -- a known variable star
10:01:33.08 +58:44:06.4 -- not a known variable star
10:01:47.99 +59:11:07.4 -- not a known variable star
10:01:48.91 +59:19:34.4 -- not a known variable star
10:02:06.48 +60:00:16.5 -- a known variable star
10:02:24.15 +59:08:11.8 -- not a known variable star
10:03:14.12 +59:34:59.3 -- not a known variable star
10:03:46.88 +59:09:42.3 -- not a known variable star
10:04:08.19 +58:18:37.8 -- a known variable star
10:04:12.93 +60:00:34.1 -- not a known variable star
10:04:53.11 +59:53:18.4 -- not a known variable star
10:05:06.18 +59:27:47.4 -- a known variable star
10:05:21.03 +59:54:08.2 -- not a known variable star
10:06:16.40 +60:17:19.1 -- not a known variable star
10:06:16.55 +59:51:03.8 -- not a known variable star
10:06:27.02 +59:31:55.2 -- not a known variable star
10:06:44.77 +60:42:28.8 -- not a known variable star
10:07:05.17 +58:02:21.7 -- a known variable star
10:07:46.74 +59:54:28.0 -- not a known variable star
10:07:54.95 +59:13:22.3 -- not a known variable star
10:08:00.96 +60:37:32.6 -- not a known variable star
10:08:15.86 +59:55:29.8 -- not a known variable star
10:08:15.86 +60:16:27.3 -- not a known variable star
10:08:20.34 +59:49:47.7 -- not a known variable star
10:08:24.15 +59:15:31.6 -- not a known variable star
10:08:25.45 +61:01:15.9 -- not a known variable star
10:08:56.14 +58:56:53.4 -- not a known variable star
10:09:14.07 +60:24:51.6 -- not a known variable star
10:09:40.01 +61:21:23.2 -- not a known variable star
10:09:43.41 +60:30:07.7 -- a known variable star
10:09:56.10 +60:07:24.8 -- not a known variable star
10:10:17.45 +61:10:40.8 -- not a known variable star
10:10:28.32 +60:22:32.5 -- not a known variable star
10:10:31.95 +60:55:20.5 -- not a known variable star
10:10:49.67 +59:25:25.9 -- not a known variable star
10:11:35.54 +61:19:40.9 -- not a known variable star
10:11:49.64 +60:47:49.0 -- not a known variable star
10:11:59.03 +60:47:46.8 -- not a known variable star
10:12:18.92 +61:11:49.1 -- not a known variable star
10:12:38.50 +61:07:06.7 -- not a known variable star
10:12:56.61 +58:55:04.6 -- not a known variable star
10:12:57.86 +60:37:56.3 -- not a known variable star
10:14:01.02 +60:38:09.5 -- not a known variable star
10:14:31.42 +59:43:49.7 -- a known variable star
10:14:35.88 +60:21:09.9 -- not a known variable star
10:14:37.24 +60:00:22.3 -- not a known variable star
10:15:15.66 +60:29:19.5 -- not a known variable star
10:15:48.11 +61:20:12.1 -- not a known variable star
10:15:54.42 +61:08:36.0 -- not a known variable star
10:15:56.25 +59:41:47.2 -- not a known variable star
10:16:12.41 +61:58:36.4 -- not a known variable star
10:16:15.69 +61:21:27.8 -- not a known variable star
10:16:18.66 +60:58:39.7 -- not a known variable star
10:16:27.10 +62:14:32.0 -- not a known variable star
10:16:33.89 +61:41:53.2 -- not a known variable star
10:16:34.37 +61:08:33.6 -- not a known variable star
10:16:35.41 +62:03:01.6 -- a known variable star
10:16:48.91 +61:27:26.6 -- not a known variable star
10:16:57.68 +60:44:25.6 -- not a known variable star
10:17:14.42 +61:11:51.6 -- not a known variable star
10:17:29.85 +61:43:41.3 -- not a known variable star
10:17:31.60 +60:25:32.1 -- a known variable star
10:17:40.97 +61:31:06.9 -- not a known variable star
10:17:43.89 +60:38:42.3 -- not a known variable star
10:18:02.30 +60:14:24.3 -- not a known variable star
10:18:02.98 +60:36:41.2 -- not a known variable star
10:18:05.01 +59:48:06.0 -- not a known variable star
10:18:28.95 +60:56:51.6 -- a known variable star
10:18:31.41 +60:59:24.5 -- not a known variable star
10:18:44.24 +61:57:16.8 -- not a known variable star
10:18:46.00 +62:03:32.2 -- not a known variable star
10:18:58.47 +61:47:58.7 -- not a known variable star
10:19:44.11 +61:26:10.0 -- not a known variable star
10:19:49.79 +61:37:46.1 -- not a known variable star
10:19:57.73 +60:01:01.0 -- not a known variable star
10:20:35.71 +62:06:21.9 -- not a known variable star
10:20:55.01 +61:30:55.6 -- not a known variable star
10:21:15.15 +60:56:22.7 -- not a known variable star
10:21:20.89 +60:12:30.3 -- a known variable star
10:21:28.39 +60:30:27.4 -- not a known variable star
10:21:38.43 +61:02:07.5 -- not a known variable star
10:22:36.19 +62:25:55.7 -- not a known variable star
10:23:42.01 +61:00:02.0 -- not a known variable star
10:23:57.27 +60:51:54.5 -- not a known variable star
10:25:03.56 +61:25:13.7 -- not a known variable star
10:25:21.16 +60:56:52.2 -- not a known variable star
10:25:26.20 +62:38:46.4 -- not a known variable star
10:25:29.57 +63:01:49.8 -- not a known variable star
10:25:43.74 +63:09:53.5 -- not a known variable star
10:25:52.64 +61:24:47.5 -- not a known variable star
10:25:54.31 +61:54:44.0 -- not a known variable star
10:25:58.84 +62:11:55.0 -- not a known variable star
10:26:23.35 +61:07:26.3 -- not a known variable star
10:26:43.74 +61:36:14.2 -- not a known variable star
10:26:55.65 +61:08:00.0 -- a known variable star
10:27:00.03 +61:15:52.5 -- not a known variable star
10:27:08.49 +62:22:09.7 -- not a known variable star
10:27:21.73 +62:06:51.9 -- not a known variable star
10:27:31.05 +63:04:43.3 -- not a known variable star
10:29:20.30 +62:23:55.3 -- not a known variable star
10:29:23.58 +62:36:56.6 -- not a known variable star
10:29:50.96 +63:22:58.8 -- not a known variable star
10:30:00.03 +62:44:35.8 -- not a known variable star
10:30:11.78 +63:08:48.5 -- a known variable star
10:31:02.44 +63:36:47.0 -- not a known variable star
10:34:12.40 +63:20:41.7 -- not a known variable star
10:34:54.53 +63:04:05.2 -- not a known variable star
10:35:25.53 +63:09:04.7 -- not a known variable star
10:37:03.90 +63:58:35.7 -- not a known variable star
10:41:02.20 +63:31:05.1 -- not a known variable star
10:47:07.03 +62:39:22.2 -- not a known variable star
10:52:45.69 +64:57:24.9 -- not a known variable star
Found 152 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
173 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 173 (excluding asteroids and hot pixels, 152 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)2461274.95645821 -observatory V36
09:46:00.93 +15:15:09.6 Mercury (-1.7mag)
12:50:32.06 -07:49:22.4 Venus (-4.5mag)
06:30:09.18 +23:38:53.4 Mars (1.3mag)
08:55:35.29 +17:52:43.3 Jupiter (-1.8mag)
00:54:48.28 +03:01:25.1 Saturn (0.5mag)
04:13:02.67 +21:00:20.4 Uranus (5.7mag)
00:15:07.53 +00:06:13.2 Neptune (7.7mag)
20:26:50.09 -23:35:14.0 Pluto (14.5mag)
17:33:06.92 -28:18:53.0 Moon (-11.0mag)
-rw-r--r-- 1 apache apache 363 Aug 22 06:03 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461274.95645821:
08:55:36.80 +17:52:36.3 Io (6.1mag)
08:55:43.94 +17:52:04.0 Europa (6.3mag)
08:55:51.81 +17:51:27.8 Ganymede (5.6mag)
08:55:16.59 +17:54:11.3 Callisto (6.9mag)
08:53:03.54 +18:00:47.4 Himalia (15.7mag)
08:55:33.30 +17:52:52.9 Thebe (16.6mag)
08:52:42.80 +17:56:38.5 Elara (17.7mag)
08:59:42.84 +17:25:56.2 Pasiphae (17.9mag)
08:57:47.98 +18:06:19.9 Carme (19.0mag)
00:54:44.17 +03:01:50.4 Titan (8.4mag)
00:54:52.74 +03:01:17.8 Rhea (9.7mag)
00:55:23.76 +03:03:07.0 Iapetus (11.1mag)
00:54:55.71 +03:01:42.5 Hyperion (14.4mag)
00:53:52.93 +02:52:49.7 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Aug 22 06:03 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461274.95645821:
20:12:17.88 -13:57:12.8 JWST
17:45:25.75 +32:26:34.5 Chandra
12:20:42.45 -62:00:50.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 22 06:03 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461274.95645821 -observatory V36
03:28:20.69 +18:26:52.8 17.5mag P/1996 R2 (Lagerkvist)
17:59:54.77 -34:28:29.2 14.2mag P/2010 H2 (Vales)
07:06:35.50 -69:29:42.0 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:13:09.82 +33:18:35.7 17.7mag C/2017 K2 (PANSTARRS)
04:21:20.23 +42:26:04.0 17.5mag P/2021 N1 (ZTF)
22:26:38.74 +30:22:07.1 17.4mag C/2022 E2 (ATLAS)
06:57:00.09 +26:16:54.1 16.8mag C/2022 N2 (PANSTARRS)
10:34:48.07 +27:50:52.4 17.0mag C/2022 QE78 (ATLAS)
09:38:22.18 +05:17:58.6 18.0mag C/2022 R6 (PANSTARRS)
15:15:41.65 -12:52:57.7 18.0mag P/2023 B1 (PANSTARRS)
20:53:19.39 +64:03:16.2 18.0mag C/2023 H5 (Lemmon)
15:36:25.30 -14:14:31.2 14.6mag C/2023 R1 (PANSTARRS)
08:23:21.69 +32:01:03.7 15.5mag C/2024 E1 (Wierzchos)
15:05:42.16 +15:30:12.5 17.8mag C/2024 G6 (ATLAS)
18:46:45.32 +43:29:22.7 13.7mag C/2024 J3 (ATLAS)
20:49:15.50 +49:41:20.2 17.5mag C/2024 R4 (PANSTARRS)
05:25:49.84 -12:53:58.4 15.3mag C/2024 T5 (ATLAS)
07:04:39.82 +21:35:20.6 17.9mag C/2025 J1 (Borisov)
10:53:25.09 +19:57:03.2 17.1mag C/2025 V2 (Rankin)
13:07:28.01 +01:20:48.8 16.9mag C/2025 Y1 (ATLAS)
16:10:37.31 +76:16:37.7 16.5mag C/2026 A2 (Bok)
03:09:55.28 +46:21:00.2 17.3mag C/2026 B2 (Sun-Gao)
11:58:56.55 +09:56:12.8 17.4mag A/2026 E1
22:12:29.11 -32:19:43.7 7.1mag 10P/Tempel
11:37:47.13 -04:19:38.7 16.3mag 29P/Schwassmann-Wachmann
11:36:36.82 -00:00:29.2 17.4mag 63P/Wild
00:51:35.58 -06:06:29.1 15.4mag 65P/Gunn
06:06:59.56 +20:14:18.5 13.7mag 78P/Gehrels
20:25:45.24 -25:00:29.1 17.5mag 84P/Giclas
03:12:03.10 +14:32:30.3 16.9mag 88P/Howell
08:30:44.19 +25:34:15.8 16.4mag 93P/Lovas
04:47:52.01 +22:27:07.8 17.2mag 112P/Urata-Niijima
06:42:52.74 +28:16:49.3 16.1mag 114P/Wiseman-Skiff
09:51:52.80 +24:04:31.4 14.9mag 123P/West-Hartley
12:12:43.60 -15:38:30.3 17.3mag 124P/Mrkos
05:56:53.22 +21:01:39.7 16.0mag 128P/Shoemaker-Holt
06:52:06.46 +18:05:40.7 17.9mag 131P/Mueller
23:59:35.25 +03:05:49.8 17.4mag 139P/Vaisala-Oterma
03:09:29.67 -18:37:22.0 12.8mag 161P/Hartley-IRAS
08:03:56.02 +38:07:17.4 16.1mag 162P/Siding Spring
11:03:09.04 +29:47:43.5 12.2mag 169P/NEAT
03:06:18.97 +09:23:28.9 17.6mag 220P/McNaught
20:16:19.60 -51:47:47.5 18.0mag 259P/Garradd
04:03:33.01 +30:51:59.4 15.3mag 260P/McNaught
07:47:35.37 +37:04:55.1 17.3mag 295P/LINEAR
15:16:14.14 +01:32:37.2 17.8mag 391P/Kowalski
09:13:48.25 +17:39:46.3 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.3K Aug 22 06:03 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
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
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
-rw-r--r-- 1 apache apache 190K Aug 22 06:03 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:27:30.457 +02:47:32.36 AT 2026xfu 2026-01-14.53 21.69
17:59:19.284 +29:24:54.02 AT 2026xft 2026-07-18.43 20.84
19:54:12.936 -24:01:35.76 AT 2026xfs 2026-05-17.56 19.77
08:44:08.771 +29:07:45.05 AT 2026xfr 2026-01-14.38 20.4
23:28:59.311 -21:41:17.71 AT 2026xfq 2026-07-19.57 21.15
20:34:55.430 -31:12:10.98 AT 2026xfp 2026-07-14.44 20
13:01:30.092 +38:12:35.50 AT 2026xfo 2026-06-23.28 20.85
23:22:05.758 +18:57:29.94 AT 2026xfn 2026-07-25.52 21.28
10:13:35.246 -20:37:42.73 AT 2026xfm 2026-01-27.58 21
21:57:25.287 +03:48:20.98 AT 2026xfl 2026-07-16.55 21.68
14:26:07.382 +33:39:52.18 AT 2026xfk 2026-06-13.34 20.9
02:09:31.559 -03:10:04.80 AT 2026xfj 2026-01-17.24 21.98
20:17:01.562 -20:06:27.94 AT 2026xfi 2026-05-20.56 20.93
21:08:09.912 -21:12:24.85 AT 2026xfh 2026-06-19.58 20.9
20:08:20.135 -25:53:36.34 AT 2026xfg 2026-07-19.45 20.74
14:51:25.078 +41:07:07.07 AT 2026xff 2026-06-13.34 21.62
22:33:15.210 +12:04:33.49 AT 2026xfe 2026-06-21.53 20.23
13:52:05.795 +29:21:47.19 AT 2026xfd 2026-04-24.32 20.92
13:30:27.613 +10:38:39.93 AT 2026xfc 2026-04-20.32 21.07
13:40:18.442 +39:30:10.71 AT 2026xfb 2026-05-24.29 20.6
-rw-r--r-- 1 apache apache 87K Aug 22 06:03 tns_transients_list.txt
