This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cyg-08-Q2b1x1_000732_TTUQ2b1x1_4080387_W1Z1EZvp
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.38 19:55:42.18 +28:34:33.7
65.37928 0.10364 galactic Vul Second-epoch detections are separated by 3.1" and 8.8 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 J298.9224+28.5830 | 19:55:42.18 +28:34:33.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.861+/-0.030 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:55:42.18 +28:34:33.7: 13.31 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:55:42.18 +28:34:33.7: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.9224+28.5830,2461199.6702,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.9224+28.5830 20260608.1702 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 06 08.1702 2461199.6702 12.14 19:56:12.03 +29:14:46.0
66.00866 0.35811 galactic Vul Second-epoch detections are separated by 1.7" and 9.1 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 J299.0467+29.2538 | 19:56:12.03 +29:14:46.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.785+/-0.032 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:12.03 +29:14:46.0: 12.97 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:12.03 +29:14:46.0: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.0467+29.2538,2461199.6702,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.0467+29.2538 20260608.1702 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 06 08.1702 2461199.6702 12.07 19:59:01.94 +32:07:51.9
68.78803 1.34326 galactic Cyg Second-epoch detections are separated by 0.9" and 8.9 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 | Gaia DR3 2033995150159336320 | 19:59:01.91 +32:07:51.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.777+/-0.027 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:01.94 +32:07:51.9: 12.97 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:01.94 +32:07:51.9: 15.84 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.97 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2033995150159336320,2461199.6702,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2033995150159336320 20260608.1702 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.09 19:59:14.54 +25:54:46.8
63.51615 -1.95558 galactic Vul Second-epoch detections are separated by 1.6" and 8.8 pix
The object was found in VSX13" Gaia DR3 1835025979809109120
Type: ROT
# Max. Min./Amp. JD0 Period
17.000 G 17.090 G 2.769270000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:14.54 +25:54:46.8: 13.14 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:14.54 +25:54:46.8: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1835025979809109120,2461199.6702,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1835025979809109120 20260608.1702 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 06 08.1702 2461199.6702 11.84 19:59:27.23 +29:50:21.7
66.88405 0.06432 galactic Cyg Second-epoch detections are separated by 0.7" and 8.9 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 | Gaia DR3 2030213830930286336 | 19:59:27.24 +29:50:21.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.253+/-0.027 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:27.23 +29:50:21.7: 12.78 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:27.23 +29:50:21.7: 12.77 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030213830930286336,2461199.6702,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030213830930286336 20260608.1702 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 06 08.1702 2461199.6702 12.21 19:58:53.23 +29:45:03.1
66.74422 0.12257 galactic Cyg Second-epoch detections are separated by 2.4" and 8.9 pix
The object was found in VSX21" Gaia DR3 2030120131903512704
Type: L
# Max. Min./Amp. JD0 Period
17.640 G 17.830 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:53.23 +29:45:03.1: 13.20 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:53.23 +29:45:03.1: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030120131903512704,2461199.6702,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030120131903512704 20260608.1702 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 06 08.1702 2461199.6702 12.34 19:55:47.57 +29:00:54.1
65.76491 0.31435 galactic Vul Second-epoch detections are separated by 0.9" and 9.0 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 | 19:55:47.57 +29:00:54.1 (user input) | T | P | (position from user input) J-Ks=0.801+/-0.030 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:55:47.57 +29:00:54.1: 13.50 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:55:47.57 +29:00:54.1: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.07 19:59:02.05 +30:00:13.6
66.97632 0.22799 galactic Cyg Second-epoch detections are separated by 0.3" and 8.9 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 | Gaia DR3 2030229739490456192 | 19:59:02.03 +30:00:13.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.983+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:02.05 +30:00:13.6: 12.98 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:02.05 +30:00:13.6: 12.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030229739490456192,2461199.6702,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030229739490456192 20260608.1702 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.28 19:56:08.65 +29:23:24.3
66.12535 0.44334 galactic Cyg Second-epoch detections are separated by 0.5" and 8.9 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 | 19:56:08.65 +29:23:24.3 (user input) | T | P | (position from user input) J-Ks=0.460+/-0.033 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:08.65 +29:23:24.3: 13.20 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:08.65 +29:23:24.3: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.15 20:00:02.15 +30:51:15.2
67.81346 0.49085 galactic Cyg Second-epoch detections are separated by 1.3" and 9.0 pix
The object was found in VSX 1" Gaia DR3 2030484173362427904
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.080 G 13.100 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:02.15 +30:51:15.2: 13.35 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:02.15 +30:51:15.2: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030484173362427904,2461199.6702,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030484173362427904 20260608.1702 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 06 08.1702 2461199.6702 12.34 19:58:57.04 +30:49:27.2
67.66562 0.67335 galactic Cyg Second-epoch detections are separated by 3.4" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.7340+30.8253 | 19:58:57.04 +30:49:27.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.331+/-0.029 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:57.04 +30:49:27.2: 13.36 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:57.04 +30:49:27.2: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.7340+30.8253,2461199.6702,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.7340+30.8253 20260608.1702 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 06 08.1702 2461199.6702 11.99 19:59:55.88 +30:43:52.0
67.69694 0.44519 galactic Cyg Second-epoch detections are separated by 0.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.9905+30.7325 | 19:59:55.82 +30:43:52.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.367+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:55.88 +30:43:52.0: 13.02 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:55.88 +30:43:52.0: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.9905+30.7325,2461199.6702,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9905+30.7325 20260608.1702 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 06 08.1702 2461199.6702 12.06 20:00:01.36 +30:43:57.1
67.70847 0.42924 galactic Cyg Second-epoch detections are separated by 0.6" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2030469192515681920 | 20:00:01.96 +30:43:22.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.321+/-0.028 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:01.36 +30:43:57.1: 13.02 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:01.36 +30:43:57.1: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2030469192515681920,2461199.6702,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2030469192515681920 20260608.1702 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 06 08.1702 2461199.6702 12.09 20:00:06.26 +30:27:25.4
67.48345 0.26936 galactic Cyg Second-epoch detections are separated by 0.7" and 8.8 pix
The object was found in VSX 9" Gaia DR3 2030269562431618048
Type: S
# Max. Min./Amp. JD0 Period
17.860 G 18.650 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:06.26 +30:27:25.4: 13.02 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:06.26 +30:27:25.4: 13.02 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030269562431618048,2461199.6702,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030269562431618048 20260608.1702 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 06 08.1702 2461199.6702 11.96 20:00:07.21 +31:41:37.9
68.53705 0.91725 galactic Cyg Second-epoch detections are separated by 1.3" and 9.0 pix
The object was found in VSX10" Gaia DR3 2030967099471834112
Type: RS
# Max. Min./Amp. JD0 Period
15.850 G 15.900 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:07.21 +31:41:37.9: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:07.21 +31:41:37.9: 14.86 +/- 0.16 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030967099471834112,2461199.6702,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030967099471834112 20260608.1702 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 06 08.1702 2461199.6702 12.09 19:56:12.07 +28:39:49.7
65.51103 0.05570 galactic Vul Second-epoch detections are separated by 2.5" and 9.4 pix
The object was found in VSX24" Gaia DR3 2028506014459391360
Type:
# Max. Min./Amp. JD0 Period
20.320 G 21.010 G 0.297642000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:12.07 +28:39:49.7: 13.02 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:12.07 +28:39:49.7: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2028506014459391360,2461199.6702,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2028506014459391360 20260608.1702 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 06 08.1702 2461199.6702 11.73 19:58:49.33 +30:22:40.3
67.27092 0.46304 galactic Cyg Second-epoch detections are separated by 0.9" and 9.0 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 | ATO J299.7045+30.3663 | 19:58:49.27 +30:22:40.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.296+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:49.33 +30:22:40.3: 12.59 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:49.33 +30:22:40.3: 12.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.7045+30.3663,2461199.6702,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.7045+30.3663 20260608.1702 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.07 20:00:35.47 +31:04:10.7
68.05929 0.50308 galactic Cyg Second-epoch detections are separated by 1.1" and 8.8 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 J300.1381+31.0651 | 20:00:35.47 +31:04:10.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.368+/-0.029 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:35.47 +31:04:10.7: 13.07 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:35.47 +31:04:10.7: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.1381+31.0651,2461199.6702,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.1381+31.0651 20260608.1702 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.87 19:58:22.20 +30:02:32.2
66.93384 0.37063 galactic Cyg Second-epoch detections are separated by 0.7" and 8.8 pix
The object was found in VSX24" ZTF J195821.95+300207.9
Type: EA
# Max. Min./Amp. JD0 Period
17.765 r Y 0.242 r 2458336.85050 1.423671400000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:22.20 +30:02:32.2: 12.85 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:22.20 +30:02:32.2: 12.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195821.95+300207.9,2461199.6702,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195821.95+300207.9 20260608.1702 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.12 19:57:27.51 +29:32:41.4
66.40633 0.27951 galactic Cyg Second-epoch detections are separated by 2.7" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.3804+29.5579 | 19:57:30.44 +29:33:00.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.301+/-0.042 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:27.51 +29:32:41.4: 13.07 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:27.51 +29:32:41.4: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.3804+29.5579,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.3804+29.5579 20260608.1702 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 06 08.1702 2461199.6702 12.39 19:57:39.51 +25:54:55.9
63.33213 -1.65060 galactic Vul Second-epoch detections are separated by 2.0" and 9.0 pix
The object was found in VSX22" Gaia DR3 2026807127254069632
Type:
# Max. Min./Amp. JD0 Period
15.570 G 16.460 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:39.51 +25:54:55.9: 13.57 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:39.51 +25:54:55.9: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2026807127254069632,2461199.6702,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026807127254069632 20260608.1702 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 06 08.1702 2461199.6702 12.35 20:01:35.30 +30:39:54.5
67.82877 0.10777 galactic Cyg Second-epoch detections are separated by 2.7" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:01:35.30 +30:39:54.5 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.465+/-0.030 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:35.30 +30:39:54.5: 13.56 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:35.30 +30:39:54.5: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.00 19:59:43.57 +29:47:33.1
66.87523 -0.01055 galactic Cyg Second-epoch detections are separated by 0.9" and 8.8 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 | 19:59:43.57 +29:47:33.1 (user input) | T | P | (position from user input) J-Ks=0.821+/-0.030 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:43.57 +29:47:33.1: 13.05 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:43.57 +29:47:33.1: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.20 19:59:42.38 +30:46:18.0
67.70603 0.50763 galactic Cyg Second-epoch detections are separated by 0.5" and 8.9 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 | Gaia DR3 2030481969990756992 | 19:59:42.32 +30:46:18.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.237+/-0.025 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:42.38 +30:46:18.0: 13.07 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:42.38 +30:46:18.0: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030481969990756992,2461199.6702,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030481969990756992 20260608.1702 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 06 08.1702 2461199.6702 12.14 19:59:02.01 +29:44:32.1
66.75353 0.09101 galactic Cyg Second-epoch detections are separated by 2.0" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2030119238563470976 | 19:59:04.60 +29:44:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.807+/-0.026 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:02.01 +29:44:32.1: 13.07 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:02.01 +29:44:32.1: 13.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030119238563470976,2461199.6702,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030119238563470976 20260608.1702 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 06 08.1702 2461199.6702 12.18 19:56:46.10 +29:12:02.6
66.03425 0.22868 galactic Vul Second-epoch detections are separated by 1.6" and 9.0 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 | ATO J299.1847+29.2120 | 19:56:46.10 +29:12:02.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.221+/-0.035 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:46.10 +29:12:02.6: 13.09 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:46.10 +29:12:02.6: 13.16 +/- 0.03 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.1847+29.2120,2461199.6702,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.1847+29.2120 20260608.1702 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 06 08.1702 2461199.6702 12.27 20:00:12.42 +30:57:13.6
67.91744 0.51202 galactic Cyg Second-epoch detections are separated by 2.2" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:12.42 +30:57:13.6 (user input) | T | P | (position from user input) J-Ks=0.285+/-0.030 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:12.42 +30:57:13.6: 13.26 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:12.42 +30:57:13.6: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.31 19:57:34.34 +25:52:41.3
63.29010 -1.65354 galactic Vul Second-epoch detections are separated by 3.8" and 8.4 pix
The object was found in VSX20" Gaia DR3 2026805585362942336
Type: L
# Max. Min./Amp. JD0 Period
18.100 G 18.350 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:34.34 +25:52:41.3: 13.41 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:34.34 +25:52:41.3: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2026805585362942336,2461199.6702,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026805585362942336 20260608.1702 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 06 08.1702 2461199.6702 12.17 19:56:00.81 +28:38:25.8
65.46975 0.07880 galactic Vul Second-epoch detections are separated by 0.3" and 9.0 pix
The object was found in VSX 1" Gaia DR3 2028508797627256832
Type: ROT
# Max. Min./Amp. JD0 Period
13.000 G 13.030 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:00.81 +28:38:25.8: 13.09 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:00.81 +28:38:25.8: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2028508797627256832,2461199.6702,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2028508797627256832 20260608.1702 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.13 19:59:59.66 +31:58:05.8
68.75643 1.08430 galactic Cyg Second-epoch detections are separated by 0.2" and 8.8 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 J300.0045+31.9674 | 19:59:59.66 +31:58:05.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.803+/-0.028 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:59.66 +31:58:05.8: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:59.66 +31:58:05.8: 15.42 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.0045+31.9674,2461199.6702,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0045+31.9674 20260608.1702 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 06 08.1702 2461199.6702 12.22 19:58:13.35 +29:44:38.5
66.66289 0.24193 galactic Cyg Second-epoch detections are separated by 1.5" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.5591+29.7368 | 19:58:13.35 +29:44:38.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.163+/-0.036 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:13.35 +29:44:38.5: 13.26 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:13.35 +29:44:38.5: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.5591+29.7368,2461199.6702,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5591+29.7368 20260608.1702 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 06 08.1702 2461199.6702 12.16 19:58:08.89 +30:27:26.6
67.26267 0.62848 galactic Cyg Second-epoch detections are separated by 1.1" and 8.9 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 | Gaia DR3 2030447816410869248 | 19:58:08.90 +30:27:27.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.697+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:08.89 +30:27:26.6: 13.12 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:08.89 +30:27:26.6: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030447816410869248,2461199.6702,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030447816410869248 20260608.1702 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 06 08.1702 2461199.6702 12.09 19:59:06.15 +30:15:35.4
67.20210 0.34966 galactic Cyg Second-epoch detections are separated by 2.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.7752+30.2598 | 19:59:06.06 +30:15:35.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.336+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:06.15 +30:15:35.4: 13.10 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:06.15 +30:15:35.4: 13.08 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.7752+30.2598,2461199.6702,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.7752+30.2598 20260608.1702 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 06 08.1702 2461199.6702 12.22 20:01:30.96 +30:19:16.6
67.52871 -0.06089 galactic Cyg Second-epoch detections are separated by 0.7" and 8.9 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 J300.3799+30.3231 | 20:01:30.96 +30:19:16.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.105+/-0.029 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:30.96 +30:19:16.6: 13.29 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:30.96 +30:19:16.6: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.3799+30.3231,2461199.6702,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.3799+30.3231 20260608.1702 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 06 08.1702 2461199.6702 12.23 19:59:31.92 +31:04:18.6
67.94183 0.69711 galactic Cyg Second-epoch detections are separated by 1.6" and 9.1 pix
The object was found in VSX 0" ZTF J195931.89+310418.7
Type: EW
# Max. Min./Amp. JD0 Period
13.504 g Y 0.274 g 2458307.84260 0.424822200000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:31.92 +31:04:18.6: 13.11 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:31.92 +31:04:18.6: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195931.89+310418.7,2461199.6702,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195931.89+310418.7 20260608.1702 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 06 08.1702 2461199.6702 11.84 19:59:31.13 +30:57:10.4
67.83912 0.63706 galactic Cyg Second-epoch detections are separated by 0.3" and 8.8 pix
The object was found in VSX 1" ASASSN-V J195931.13+305711.0
Type: SR
# Max. Min./Amp. JD0 Period
13.960 g Y 0.190 g 2459467.82000 664.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:31.13 +30:57:10.4: 12.90 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:31.13 +30:57:10.4: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195931.13+305711.0,2461199.6702,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195931.13+305711.0 20260608.1702 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 06 08.1702 2461199.6702 12.24 20:01:38.22 +31:27:49.9
68.51210 0.52147 galactic Cyg Second-epoch detections are separated by 1.2" and 8.9 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 | Gaia DR3 2030902228289582464 | 20:01:41.15 +31:27:55.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5) J-Ks=0.896+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:38.22 +31:27:49.9: 13.12 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:38.22 +31:27:49.9: 15.04 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030902228289582464,2461199.6702,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030902228289582464 20260608.1702 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.73 20:00:57.01 +25:59:35.3
63.78618 -2.24015 galactic Vul Second-epoch detections are separated by 1.7" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.2332+25.9913 | 20:00:57.07 +25:59:37.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.901+/-0.029 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:57.01 +25:59:35.3: 12.69 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:57.01 +25:59:35.3: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.2332+25.9913,2461199.6702,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.2332+25.9913 20260608.1702 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.24 19:56:49.81 +28:52:07.3
65.75772 0.04441 galactic Vul Second-epoch detections are separated by 1.3" and 8.8 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 J299.2101+28.8597 | 19:56:49.76 +28:52:06.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.319+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:49.81 +28:52:07.3: 13.13 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:49.81 +28:52:07.3: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.2101+28.8597,2461199.6702,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.2101+28.8597 20260608.1702 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.14 19:57:47.82 +29:07:01.6
66.07991 -0.00657 galactic Vul Second-epoch detections are separated by 2.9" and 8.8 pix
The object was found in VSX 3" ASASSN-V J195747.65+290659.8
Type: SR
# Max. Min./Amp. JD0 Period
13.920 V 14.300 V 2458209.85010 81.857302800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:47.82 +29:07:01.6: 13.13 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:47.82 +29:07:01.6: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195747.65+290659.8,2461199.6702,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195747.65+290659.8 20260608.1702 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 06 08.1702 2461199.6702 12.13 20:02:12.23 +30:49:33.0
68.03512 0.08069 galactic Cyg Second-epoch detections are separated by 2.6" and 9.1 pix
The object was found in VSX12" ZTF J200212.87+304924.9
Type: EA
# Max. Min./Amp. JD0 Period
17.738 g Y 0.337 g 2458632.97960 3.445786700000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:12.23 +30:49:33.0: 13.11 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:12.23 +30:49:33.0: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200212.87+304924.9,2461199.6702,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J200212.87+304924.9 20260608.1702 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 06 08.1702 2461199.6702 11.99 19:57:14.83 +28:55:17.9
65.85044 -0.00595 galactic Vul Second-epoch detections are separated by 1.1" and 8.9 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 | 19:57:14.83 +28:55:17.9 (user input) | T | P | (position from user input) J-Ks=0.233+/-0.033 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:14.83 +28:55:17.9: 12.94 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:14.83 +28:55:17.9: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.22 20:02:44.28 +30:09:48.8
67.53484 -0.36829 galactic Cyg Second-epoch detections are separated by 1.8" and 9.0 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 | 20:02:44.28 +30:09:48.8 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.028 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:44.28 +30:09:48.8: 13.13 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:44.28 +30:09:48.8: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.90 20:00:16.53 +29:17:15.9
66.50878 -0.37769 galactic Vul Second-epoch detections are separated by 2.3" and 8.5 pix
The object was found in VSX 3" ASASSN-V J200016.44+291713.5
Type: SR
# Max. Min./Amp. JD0 Period
14.490 g Y 0.540 g 2458678.63000 54.410000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:16.53 +29:17:15.9: 12.70 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:16.53 +29:17:15.9: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200016.44+291713.5,2461199.6702,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200016.44+291713.5 20260608.1702 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.98 20:02:18.84 +25:53:56.9
63.86827 -2.55017 galactic Vul Second-epoch detections are separated by 1.7" and 8.8 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 1834979113126424960 | 20:02:18.83 +25:53:55.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.317+/-9.995 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:18.84 +25:53:56.9: 12.95 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:18.84 +25:53:56.9: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1834979113126424960,2461199.6702,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834979113126424960 20260608.1702 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.07 20:01:36.08 +31:04:07.4
68.17274 0.31890 galactic Cyg Second-epoch detections are separated by 0.9" and 8.8 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 J300.4065+31.0780 | 20:01:36.08 +31:04:07.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.840+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:36.08 +31:04:07.4: 12.97 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:36.08 +31:04:07.4: 14.13 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.4065+31.0780,2461199.6702,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.4065+31.0780 20260608.1702 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.67 19:57:05.99 +25:58:00.7
63.31054 -1.51665 galactic Vul Second-epoch detections are separated by 0.7" and 9.1 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 J299.2747+25.9669 | 19:57:05.92 +25:58:00.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M6 (LAMOST DR5) J-Ks=1.616+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:05.99 +25:58:00.7: 12.72 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:05.99 +25:58:00.7: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.2747+25.9669,2461199.6702,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.2747+25.9669 20260608.1702 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.79 20:00:15.48 +30:25:29.9
67.47361 0.22431 galactic Cyg Second-epoch detections are separated by 0.6" and 8.9 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 J300.0580+30.4151 | 20:00:15.44 +30:25:30.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5) J-Ks=1.149+/-0.040 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:15.48 +30:25:29.9: 12.72 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:15.48 +30:25:29.9: 12.77 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.0580+30.4151,2461199.6702,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0580+30.4151 20260608.1702 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.28 19:53:33.24 +26:25:49.4
63.29573 -0.59617 galactic Vul Second-epoch detections are separated by 2.8" and 9.2 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 | 19:53:33.24 +26:25:49.4 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.027 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:53:33.24 +26:25:49.4: 13.31 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:53:33.24 +26:25:49.4: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.44 20:00:13.59 +31:31:48.2
68.40966 0.81180 galactic Cyg Second-epoch detections are separated by 1.3" and 9.1 pix
The object was found in VSX 0" ASASSN-V J200013.59+313148.4
Type: SRS
# Max. Min./Amp. JD0 Period
14.000 V 14.090 V 2457206.96600 20.464000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:13.59 +31:31:48.2: 13.59 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:13.59 +31:31:48.2: 15.25 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.72 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J200013.59+313148.4,2461199.6702,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200013.59+313148.4 20260608.1702 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 06 08.1702 2461199.6702 11.51 20:00:26.88 +30:20:56.8
67.43070 0.14953 galactic Cyg Second-epoch detections are separated by 0.9" and 9.0 pix
The object was found in VSX17" Gaia DR3 2030264923865292544
Type:
# Max. Min./Amp. JD0 Period
16.170 G 16.990 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:26.88 +30:20:56.8: 12.42 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:26.88 +30:20:56.8: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030264923865292544,2461199.6702,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030264923865292544 20260608.1702 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.56 19:58:28.50 +25:46:25.3
63.30699 -1.88133 galactic Vul Second-epoch detections are separated by 0.5" and 8.9 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 J299.6209+25.7685 | 19:58:28.50 +25:46:24.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.765+/-0.031 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:28.50 +25:46:25.3: 12.43 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:28.50 +25:46:25.3: 12.50 +/- 0.02 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.6209+25.7685,2461199.6702,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6209+25.7685 20260608.1702 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.53 19:59:05.35 +30:17:17.9
67.22484 0.36704 galactic Cyg Second-epoch detections are separated by 1.6" and 8.9 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 J299.7598+30.2738 | 19:59:04.97 +30:16:41.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.266+/-0.025 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:05.35 +30:17:17.9: 12.41 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:05.35 +30:17:17.9: 12.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.42 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.7598+30.2738,2461199.6702,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.7598+30.2738 20260608.1702 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.49 19:58:56.24 +30:04:00.0
67.01889 0.27880 galactic Cyg Second-epoch detections are separated by 1.4" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2030233446010615936 | 19:58:56.22 +30:03:59.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.720+/-0.028 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:56.24 +30:04:00.0: 12.42 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:56.24 +30:04:00.0: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030233446010615936,2461199.6702,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030233446010615936 20260608.1702 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.51 19:57:52.09 +25:49:28.0
63.27896 -1.73833 galactic Vul Second-epoch detections are separated by 0.7" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1834651394268531456 | 19:57:52.20 +25:49:28.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.398+/-0.030 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:52.09 +25:49:28.0: 12.39 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:52.09 +25:49:28.0: 12.51 +/- 0.02 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1834651394268531456,2461199.6702,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834651394268531456 20260608.1702 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.76 19:54:59.59 +25:52:13.3
62.98234 -1.16163 galactic Vul Second-epoch detections are separated by 1.6" and 8.8 pix
The object was found in VSX13" Gaia DR3 2026795002573294848
Type: ROT
# Max. Min./Amp. JD0 Period
14.880 G 14.910 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:59.59 +25:52:13.3: 12.73 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:59.59 +25:52:13.3: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2026795002573294848,2461199.6702,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026795002573294848 20260608.1702 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 06 08.1702 2461199.6702 12.24 19:57:33.00 +29:37:15.8
66.48174 0.30229 galactic Cyg Second-epoch detections are separated by 3.9" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2030124048927449856 | 19:57:34.63 +29:37:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:33.00 +29:37:15.8: 13.27 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:33.00 +29:37:15.8: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030124048927449856,2461199.6702,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030124048927449856 20260608.1702 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.80 20:01:17.30 +25:52:51.8
63.73095 -2.36384 galactic Vul Second-epoch detections are separated by 1.4" and 8.7 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 | 20:01:17.30 +25:52:51.8 (user input) | T | P | (position from user input) J-Ks=0.697+/-0.029 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:17.30 +25:52:51.8: 12.70 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:17.30 +25:52:51.8: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.27 20:01:50.92 +25:46:33.9
63.70831 -2.52633 galactic Vul Second-epoch detections are separated by 2.3" and 9.0 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 | 20:01:50.92 +25:46:33.9 (user input) | T | P | (position from user input) J-Ks=1.144+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:50.92 +25:46:33.9: 13.31 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:50.92 +25:46:33.9: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.98 19:58:22.33 +29:57:37.3
66.86426 0.32738 galactic Cyg Second-epoch detections are separated by 1.2" and 8.9 pix
The object was found in VSX 0" ASASSN-V J195822.35+295736.9
Type: SR
# Max. Min./Amp. JD0 Period
13.580 V 13.680 V 2458180.00000 790.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:22.33 +29:57:37.3: 12.98 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:22.33 +29:57:37.3: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J195822.35+295736.9,2461199.6702,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195822.35+295736.9 20260608.1702 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.85 20:02:05.32 +25:52:26.7
63.82015 -2.52040 galactic Vul Second-epoch detections are separated by 1.3" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1834978632090089088 | 20:02:05.15 +25:52:26.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.934+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:05.32 +25:52:26.7: 12.72 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:05.32 +25:52:26.7: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1834978632090089088,2461199.6702,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834978632090089088 20260608.1702 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 06 08.1702 2461199.6702 11.88 20:00:49.34 +30:03:56.3
67.23247 -0.06865 galactic Cyg Second-epoch detections are separated by 1.3" and 9.1 pix
The object was found in VSX23" Gaia DR3 2030244204941885952
Type: ROT
# Max. Min./Amp. JD0 Period
14.810 G 14.860 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:49.34 +30:03:56.3: 12.69 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:49.34 +30:03:56.3: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030244204941885952,2461199.6702,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030244204941885952 20260608.1702 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.21 19:53:31.30 +26:20:57.6
63.22249 -0.63165 galactic Vul Second-epoch detections are separated by 1.7" and 8.8 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 | 19:53:31.30 +26:20:57.6 (user input) | T | P | (position from user input) J-Ks=0.482+/-0.029 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:53:31.30 +26:20:57.6: 13.15 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:53:31.30 +26:20:57.6: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.18 20:01:41.88 +26:12:07.5
64.05246 -2.27259 galactic Vul Second-epoch detections are separated by 1.1" and 8.9 pix
The object was found in VSX 2" Gaia DR3 1835050654422762240
Type: ROT
# Max. Min./Amp. JD0 Period
13.110 G 13.140 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:41.88 +26:12:07.5: 13.16 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:41.88 +26:12:07.5: 13.25 +/- 0.03 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1835050654422762240,2461199.6702,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1835050654422762240 20260608.1702 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 06 08.1702 2461199.6702 11.87 19:58:19.70 +25:49:11.5
63.32912 -1.82906 galactic Vul Second-epoch detections are separated by 2.0" and 8.7 pix
The object was found in VSX23" ZTF J195821.25+254920.2
Type: RS:
# Max. Min./Amp. JD0 Period
16.927 r Y 0.083 r 2458293.82250 0.187899400000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:19.70 +25:49:11.5: 12.76 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:19.70 +25:49:11.5: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195821.25+254920.2,2461199.6702,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195821.25+254920.2 20260608.1702 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.53 19:59:39.56 +25:55:00.5
63.56857 -2.03344 galactic Vul Second-epoch detections are separated by 1.5" and 8.8 pix
The object was found in VSX 2" ASASSN-V J195939.54+255458.7
Type: SR
# Max. Min./Amp. JD0 Period
13.480 V 13.650 V 2457241.00000 527.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:39.56 +25:55:00.5: 12.38 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:39.56 +25:55:00.5: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J195939.54+255458.7,2461199.6702,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195939.54+255458.7 20260608.1702 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.96 20:01:56.56 +33:35:50.9
70.35698 1.59575 galactic Cyg Second-epoch detections are separated by 0.7" and 8.7 pix
The object was found in VSX 1" ASASSN-V J200156.62+333551.6
Type: SR
# Max. Min./Amp. JD0 Period
13.400 V 13.800 V 2457453.10000 227.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:56.56 +33:35:50.9: 12.93 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:56.56 +33:35:50.9: 15.34 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.93 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200156.62+333551.6,2461199.6702,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200156.62+333551.6 20260608.1702 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 06 08.1702 2461199.6702 12.23 20:00:51.93 +25:49:06.9
63.62764 -2.31590 galactic Vul Second-epoch detections are separated by 3.4" and 9.2 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 | 20:00:51.93 +25:49:06.9 (user input) | T | P | (position from user input) J-Ks=0.473+/-0.029 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:51.93 +25:49:06.9: 13.31 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:51.93 +25:49:06.9: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.96 20:00:49.22 +32:15:28.5
69.09482 1.08812 galactic Cyg Second-epoch detections are separated by 3.4" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2034084008768987904 | 20:00:49.17 +32:15:27.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.782+/-0.026 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:49.22 +32:15:28.5: 12.98 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:49.22 +32:15:28.5: 15.63 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2034084008768987904,2461199.6702,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034084008768987904 20260608.1702 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 06 08.1702 2461199.6702 11.94 19:58:45.81 +25:54:26.8
63.45502 -1.86674 galactic Vul Second-epoch detections are separated by 1.2" and 9.0 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 | ATO J299.6783+25.9108 | 19:58:45.81 +25:54:26.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.857+/-0.033 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:45.81 +25:54:26.8: 12.95 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:45.81 +25:54:26.8: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.6783+25.9108,2461199.6702,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6783+25.9108 20260608.1702 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.93 19:57:41.93 +25:45:47.4
63.20677 -1.73775 galactic Vul Second-epoch detections are separated by 2.0" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1834650019878994688 | 19:57:44.50 +25:46:07.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F4 (LAMOST DR5)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:41.93 +25:45:47.4: 12.90 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:41.93 +25:45:47.4: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1834650019878994688,2461199.6702,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834650019878994688 20260608.1702 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.97 19:56:30.01 +25:46:24.1
63.07504 -1.50197 galactic Vul Second-epoch detections are separated by 2.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2026800770699685248 | 19:56:30.64 +25:45:55.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.605+/-0.033 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:30.01 +25:46:24.1: 12.95 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:30.01 +25:46:24.1: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2026800770699685248,2461199.6702,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026800770699685248 20260608.1702 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 06 08.1702 2461199.6702 11.94 20:00:48.41 +30:37:37.6
67.70769 0.23040 galactic Cyg Second-epoch detections are separated by 0.5" and 8.8 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 2030278358524077568 | 20:00:48.37 +30:37:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.140+/-0.030 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:48.41 +30:37:37.6: 12.96 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:48.41 +30:37:37.6: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030278358524077568,2461199.6702,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030278358524077568 20260608.1702 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.46 20:01:15.44 +30:23:20.1
67.55662 0.02224 galactic Cyg Second-epoch detections are separated by 1.3" and 9.1 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 J300.3251+30.3900 | 20:01:15.41 +30:23:20.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.230+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:15.44 +30:23:20.1: 12.36 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:15.44 +30:23:20.1: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J300.3251+30.3900,2461199.6702,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.3251+30.3900 20260608.1702 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.04 19:59:02.39 +30:43:30.7
67.59132 0.60514 galactic Cyg Second-epoch detections are separated by 1.0" and 8.8 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 2030476334993669376 | 19:59:02.38 +30:43:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.851+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:02.39 +30:43:30.7: 12.94 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:02.39 +30:43:30.7: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030476334993669376,2461199.6702,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030476334993669376 20260608.1702 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 06 08.1702 2461199.6702 11.94 19:58:12.63 +30:30:42.9
67.31618 0.64553 galactic Cyg Second-epoch detections are separated by 1.4" and 8.9 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 J299.5667+30.5105 | 19:58:12.54 +30:30:42.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.882+/-0.027 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:12.63 +30:30:42.9: 12.95 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:12.63 +30:30:42.9: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.5667+30.5105,2461199.6702,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5667+30.5105 20260608.1702 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.02 20:02:07.55 +30:33:14.9
67.79585 -0.04911 galactic Cyg Second-epoch detections are separated by 1.3" and 8.7 pix
The object was found in VSX 1" Gaia DR3 2030637069847520512
Type: ROT
# Max. Min./Amp. JD0 Period
12.620 G 12.660 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:07.55 +30:33:14.9: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:07.55 +30:33:14.9: 13.34 +/- 0.03 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030637069847520512,2461199.6702,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030637069847520512 20260608.1702 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 06 08.1702 2461199.6702 12.29 19:59:56.37 +32:24:56.1
69.13093 1.32931 galactic Cyg Second-epoch detections are separated by 1.2" and 8.7 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 | 19:59:56.37 +32:24:56.1 (user input) | T | P | (position from user input) J-Ks=1.128+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:56.37 +32:24:56.1: 13.32 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:56.37 +32:24:56.1: 14.37 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.12 19:54:49.28 +26:12:09.2
63.24687 -0.95697 galactic Vul Second-epoch detections are separated by 2.1" and 8.8 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 J298.7040+26.2000 | 19:54:49.28 +26:12:09.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.391+/-0.033 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:49.28 +26:12:09.2: 12.95 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:49.28 +26:12:09.2: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.7040+26.2000,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.7040+26.2000 20260608.1702 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 06 08.1702 2461199.6702 12.02 20:03:09.52 +30:01:38.4
67.46781 -0.51776 galactic Cyg Second-epoch detections are separated by 1.1" and 8.9 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 | Gaia DR3 2030186029571679232 | 20:03:09.49 +30:01:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.357+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:03:09.52 +30:01:38.4: 12.94 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:03:09.52 +30:01:38.4: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030186029571679232,2461199.6702,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030186029571679232 20260608.1702 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 06 08.1702 2461199.6702 12.11 19:58:21.53 +30:05:01.1
66.96783 0.39432 galactic Cyg Second-epoch detections are separated by 0.7" and 8.9 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 J299.5804+30.0863 | 19:58:21.53 +30:05:01.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.699+/-0.030 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:21.53 +30:05:01.1: 13.15 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:21.53 +30:05:01.1: 13.05 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.5804+30.0863,2461199.6702,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5804+30.0863 20260608.1702 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 06 08.1702 2461199.6702 11.75 19:58:42.19 +25:50:16.2
63.38855 -1.89158 galactic Vul Second-epoch detections are separated by 0.7" and 9.0 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 | ATO J299.6897+25.8389 | 19:58:42.19 +25:50:16.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.443+/-0.032 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:42.19 +25:50:16.2: 12.71 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:42.19 +25:50:16.2: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.6897+25.8389,2461199.6702,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6897+25.8389 20260608.1702 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.96 20:00:09.95 +30:47:52.9
67.78036 0.43755 galactic Cyg Second-epoch detections are separated by 0.6" and 8.9 pix
The object was found in VSX23" Gaia DR3 2030472044373924224
Type: L
# Max. Min./Amp. JD0 Period
14.300 G 14.590 G M
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:09.95 +30:47:52.9: 12.96 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:09.95 +30:47:52.9: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030472044373924224,2461199.6702,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030472044373924224 20260608.1702 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 06 08.1702 2461199.6702 11.96 19:58:14.32 +29:22:03.3
66.34382 0.04213 galactic Cyg Second-epoch detections are separated by 0.6" and 8.9 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 | 19:58:14.32 +29:22:03.3 (user input) | T | P | (position from user input) J-Ks=0.817+/-0.031 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:14.32 +29:22:03.3: 12.92 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:14.32 +29:22:03.3: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.20 19:58:50.92 +30:38:18.2
67.49584 0.59466 galactic Cyg Second-epoch detections are separated by 0.9" and 8.8 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 | 19:58:50.92 +30:38:18.2 (user input) | T | P | (position from user input) J-Ks=0.816+/-0.026 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:50.92 +30:38:18.2: 13.15 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:50.92 +30:38:18.2: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.18 19:59:55.54 +31:12:18.6
68.09955 0.69550 galactic Cyg Second-epoch detections are separated by 0.3" and 8.9 pix
The object was found in VSX11" Gaia DR3 2030915349386140032
Type: E
# Max. Min./Amp. JD0 Period
17.550 G 17.680 G 0.660900000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:55.54 +31:12:18.6: 13.15 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:55.54 +31:12:18.6: 14.02 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030915349386140032,2461199.6702,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030915349386140032 20260608.1702 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 06 08.1702 2461199.6702 11.43 19:58:06.90 +25:43:31.1
63.22335 -1.83746 galactic Vul Second-epoch detections are separated by 0.7" and 8.9 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 J299.5362+25.7250 | 19:58:06.85 +25:43:30.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-0.034 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:06.90 +25:43:31.1: 12.32 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:06.90 +25:43:31.1: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.37 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.5362+25.7250,2461199.6702,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5362+25.7250 20260608.1702 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.11 20:01:44.85 +30:36:59.9
67.80573 0.05305 galactic Cyg Second-epoch detections are separated by 1.2" and 9.0 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 | ATO J300.4350+30.6223 | 20:01:44.78 +30:37:00.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.405+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:44.85 +30:36:59.9: 13.14 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:44.85 +30:36:59.9: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.4350+30.6223,2461199.6702,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.4350+30.6223 20260608.1702 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 06 08.1702 2461199.6702 12.03 19:59:22.85 +30:11:08.3
67.17048 0.25955 galactic Cyg Second-epoch detections are separated by 4.6" and 9.4 pix
The object was found in VSX 1" ASASSN-V J195922.82+301107.6
Type: SR
# Max. Min./Amp. JD0 Period
13.650 V 14.010 V 2458323.75250 89.628000800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:22.85 +30:11:08.3: 13.15 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:22.85 +30:11:08.3: 13.16 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195922.82+301107.6,2461199.6702,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195922.82+301107.6 20260608.1702 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 06 08.1702 2461199.6702 12.12 19:59:35.27 +30:06:32.3
67.12873 0.18121 galactic Cyg Second-epoch detections are separated by 1.5" and 9.0 pix
The object was found in VSX21" Gaia DR3 2030236817577361536
Type: L
# Max. Min./Amp. JD0 Period
19.700 G 20.370 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:35.27 +30:06:32.3: 13.13 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:35.27 +30:06:32.3: 12.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030236817577361536,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030236817577361536 20260608.1702 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 06 08.1702 2461199.6702 11.77 20:00:15.72 +25:46:33.8
63.51994 -2.22274 galactic Vul Second-epoch detections are separated by 0.6" and 9.0 pix
The object was found in VSX10" Gaia DR3 1834967602619287040
Type: ROT
# Max. Min./Amp. JD0 Period
18.370 G 19.120 G 6.774400000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:15.72 +25:46:33.8: 12.68 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:15.72 +25:46:33.8: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1834967602619287040,2461199.6702,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834967602619287040 20260608.1702 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.12 20:01:44.41 +33:21:00.5
70.12467 1.50076 galactic Cyg Second-epoch detections are separated by 2.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:01:44.41 +33:21:00.5 (user input) | T | P | (position from user input) J-Ks=11.893+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:44.41 +33:21:00.5: 13.13 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:44.41 +33:21:00.5: 15.25 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.12 19:57:12.81 +29:25:39.3
66.27847 0.26391 galactic Cyg Second-epoch detections are separated by 0.5" and 8.9 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 J299.2811+29.4233 | 19:57:10.32 +29:25:15.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.076+/-0.030 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:12.81 +29:25:39.3: 13.12 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:12.81 +29:25:39.3: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.2811+29.4233,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.2811+29.4233 20260608.1702 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 06 08.1702 2461199.6702 12.11 19:58:57.46 +25:49:51.1
63.41258 -1.94403 galactic Vul Second-epoch detections are separated by 0.5" and 8.9 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 | 19:58:57.46 +25:49:51.1 (user input) | T | P | (position from user input) J-Ks=1.916+/- (Very red!)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:57.46 +25:49:51.1: 13.16 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:57.46 +25:49:51.1: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.49 19:58:19.27 +26:01:55.4
63.50932 -1.71686 galactic Vul Second-epoch detections are separated by 0.8" and 9.0 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 | ATO J299.5770+26.0341 | 19:58:19.18 +26:01:55.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.311+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:19.27 +26:01:55.4: 12.32 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:19.27 +26:01:55.4: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.5770+26.0341,2461199.6702,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5770+26.0341 20260608.1702 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.21 19:56:31.44 +29:05:41.9
65.91618 0.21927 galactic Vul Second-epoch detections are separated by 3.3" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.1275+29.0963 | 19:56:31.44 +29:05:41.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:31.44 +29:05:41.9: 13.14 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:31.44 +29:05:41.9: 13.21 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.1275+29.0963,2461199.6702,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.1275+29.0963 20260608.1702 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 06 08.1702 2461199.6702 12.24 20:00:30.25 +31:40:36.0
68.56545 0.83874 galactic Cyg Second-epoch detections are separated by 1.0" and 8.8 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 | 20:00:30.25 +31:40:36.0 (user input) | T | P | (position from user input) J-Ks=0.833+/-0.030 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:30.25 +31:40:36.0: 13.14 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:30.25 +31:40:36.0: 14.67 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.21 19:56:49.55 +28:54:45.5
65.79475 0.06809 galactic Vul Second-epoch detections are separated by 0.6" and 8.9 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 J299.2078+28.9033 | 19:56:49.55 +28:54:45.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.811+/-0.030 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:49.55 +28:54:45.5: 13.14 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:49.55 +28:54:45.5: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.2078+28.9033,2461199.6702,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.2078+28.9033 20260608.1702 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 06 08.1702 2461199.6702 12.05 20:01:44.93 +25:46:13.2
63.69154 -2.51028 galactic Vul Second-epoch detections are separated by 0.7" and 9.0 pix
The object was found in VSX15" Gaia DR3 1834976368667207296
Type: ROT
# Max. Min./Amp. JD0 Period
16.420 G 16.480 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:44.93 +25:46:13.2: 12.94 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:44.93 +25:46:13.2: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1834976368667207296,2461199.6702,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834976368667207296 20260608.1702 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 06 08.1702 2461199.6702 11.99 19:59:07.44 +29:36:00.5
66.64283 -0.00025 galactic Cyg Second-epoch detections are separated by 0.3" and 8.9 pix
The object was found in VSX10" Gaia DR3 2030114355153164160
Type: RS
# Max. Min./Amp. JD0 Period
17.290 G 17.420 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:07.44 +29:36:00.5: 12.92 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:07.44 +29:36:00.5: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030114355153164160,2461199.6702,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030114355153164160 20260608.1702 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 06 08.1702 2461199.6702 12.06 20:02:10.36 +25:45:33.1
63.73254 -2.59719 galactic Vul Second-epoch detections are separated by 2.5" and 8.8 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 J300.5524+25.7570 | 20:02:10.36 +25:45:33.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.352+/-0.028 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:10.36 +25:45:33.1: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:10.36 +25:45:33.1: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.5524+25.7570,2461199.6702,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.5524+25.7570 20260608.1702 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 06 08.1702 2461199.6702 11.97 20:00:31.74 +31:51:06.3
68.71706 0.92649 galactic Cyg Second-epoch detections are separated by 1.2" and 9.0 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 | ATO J300.1258+31.8549 | 20:00:31.74 +31:51:06.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A9V (LAMOST DR5) J-Ks=0.265+/-0.030 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:31.74 +31:51:06.3: 12.93 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:31.74 +31:51:06.3: 15.70 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.93 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.1258+31.8549,2461199.6702,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.1258+31.8549 20260608.1702 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 06 08.1702 2461199.6702 12.01 19:58:26.78 +30:07:56.3
67.01920 0.40365 galactic Cyg Second-epoch detections are separated by 0.6" and 8.8 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 J299.6014+30.1332 | 19:58:26.78 +30:07:56.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.362+/-0.032 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:26.78 +30:07:56.3: 12.94 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:26.78 +30:07:56.3: 12.89 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.6014+30.1332,2461199.6702,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6014+30.1332 20260608.1702 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 06 08.1702 2461199.6702 11.43 19:54:35.97 +25:52:08.6
62.93548 -1.08647 galactic Vul Second-epoch detections are separated by 0.5" and 9.0 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 | ATO J298.6498+25.8689 | 19:54:35.96 +25:52:08.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5) J-Ks=0.173+/-0.028 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:35.97 +25:52:08.6: 12.30 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:35.97 +25:52:08.6: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J298.6498+25.8689,2461199.6702,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.6498+25.8689 20260608.1702 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.04 20:00:35.55 +31:47:44.5
68.67652 0.88549 galactic Cyg Second-epoch detections are separated by 2.1" and 8.8 pix
The object was found in VSX 1" Gaia DR3 2030969367214720512
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.850 G 12.880 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:35.55 +31:47:44.5: 13.15 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:35.55 +31:47:44.5: 15.56 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.15 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030969367214720512,2461199.6702,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030969367214720512 20260608.1702 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 06 08.1702 2461199.6702 11.46 19:53:28.93 +25:57:40.5
62.88507 -0.82363 galactic Vul Second-epoch detections are separated by 1.7" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2026852074100727424 | 19:53:28.88 +25:57:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.238+/-0.031 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:53:28.93 +25:57:40.5: 12.30 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:53:28.93 +25:57:40.5: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2026852074100727424,2461199.6702,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026852074100727424 20260608.1702 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.94 19:59:21.96 +25:45:38.9
63.40102 -2.05902 galactic Vul Second-epoch detections are separated by 2.7" and 9.0 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 | ATO J299.8391+25.7573 | 19:59:21.96 +25:45:38.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.789+/-0.028 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:21.96 +25:45:38.9: 12.90 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:21.96 +25:45:38.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.8391+25.7573,2461199.6702,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.8391+25.7573 20260608.1702 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.01 19:59:20.79 +31:19:32.0
68.13699 0.86405 galactic Cyg Second-epoch detections are separated by 2.9" and 8.9 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 J299.8260+31.3298 | 19:59:20.76 +31:19:31.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.764+/-0.030 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:20.79 +31:19:32.0: 12.92 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:20.79 +31:19:32.0: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.8260+31.3298,2461199.6702,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.8260+31.3298 20260608.1702 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 06 08.1702 2461199.6702 12.29 19:57:48.62 +29:59:35.9
66.82878 0.44834 galactic Cyg Second-epoch detections are separated by 2.5" and 9.1 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 J299.4554+29.9931 | 19:57:48.62 +29:59:35.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:48.62 +29:59:35.9: 13.34 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:48.62 +29:59:35.9: 13.37 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.4554+29.9931,2461199.6702,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.4554+29.9931 20260608.1702 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 06 08.1702 2461199.6702 12.22 19:59:03.28 +30:47:12.5
67.64546 0.63472 galactic Cyg Second-epoch detections are separated by 1.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:59:03.28 +30:47:12.5 (user input) | T | P | (position from user input) J-Ks=0.325+/-0.045 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:03.28 +30:47:12.5: 13.27 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:03.28 +30:47:12.5: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.38 20:00:13.73 +32:19:46.3
69.08985 1.23209 galactic Cyg Second-epoch detections are separated by 2.7" and 8.9 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 | 20:00:13.73 +32:19:46.3 (user input) | T | P | (position from user input) J-Ks=0.832+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:13.73 +32:19:46.3: 13.40 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:13.73 +32:19:46.3: 15.94 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.40 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.01 20:00:55.43 +31:15:31.2
68.25743 0.54231 galactic Cyg Second-epoch detections are separated by 1.9" and 9.1 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 J300.2277+31.2581 | 20:00:55.43 +31:15:31.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:55.43 +31:15:31.2: 12.98 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:55.43 +31:15:31.2: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.2277+31.2581,2461199.6702,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.2277+31.2581 20260608.1702 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 06 08.1702 2461199.6702 12.02 19:53:25.38 +26:18:02.4
63.16938 -0.63772 galactic Vul Second-epoch detections are separated by 1.5" and 8.8 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 2027054590401860480 | 19:53:25.24 +26:18:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.957+/-0.027 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:53:25.38 +26:18:02.4: 12.93 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:53:25.38 +26:18:02.4: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2027054590401860480,2461199.6702,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2027054590401860480 20260608.1702 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 06 08.1702 2461199.6702 11.87 19:57:49.50 +25:59:41.9
63.41947 -1.64112 galactic Vul Second-epoch detections are separated by 2.0" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2026808604720047488 | 19:57:49.44 +25:59:40.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5) J-Ks=1.469+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:49.50 +25:59:41.9: 12.91 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:49.50 +25:59:41.9: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2026808604720047488,2461199.6702,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026808604720047488 20260608.1702 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.95 20:00:22.78 +31:12:04.9
68.14740 0.61095 galactic Cyg Second-epoch detections are separated by 1.0" and 8.9 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 J300.0833+31.2070 | 20:00:22.78 +31:12:04.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.157+/-0.027 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:22.78 +31:12:04.9: 12.91 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:22.78 +31:12:04.9: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.0833+31.2070,2461199.6702,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0833+31.2070 20260608.1702 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 06 08.1702 2461199.6702 12.02 20:01:05.47 +30:29:15.8
67.62160 0.10484 galactic Cyg Second-epoch detections are separated by 2.1" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.2814+30.4985 | 20:01:05.55 +30:29:16.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.414+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:05.47 +30:29:15.8: 12.90 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:05.47 +30:29:15.8: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.2814+30.4985,2461199.6702,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.2814+30.4985 20260608.1702 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 06 08.1702 2461199.6702 12.23 19:57:29.34 +28:52:33.4
65.83903 -0.07494 galactic Vul Second-epoch detections are separated by 1.9" and 8.8 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 | 19:57:29.34 +28:52:33.4 (user input) | T | P | (position from user input) J-Ks=10.645+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:29.34 +28:52:33.4: 13.15 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:29.34 +28:52:33.4: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.17 19:59:33.89 +31:00:18.8
67.88883 0.65615 galactic Cyg Second-epoch detections are separated by 4.1" and 9.0 pix
The object was found in VSX19" ZTF J195932.89+310033.1
Type: SR
# Max. Min./Amp. JD0 Period
17.434 r Y 0.097 r 2458637.81460 26.842987600000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:33.89 +31:00:18.8: 13.12 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:33.89 +31:00:18.8: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195932.89+310033.1,2461199.6702,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195932.89+310033.1 20260608.1702 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.10 19:59:48.91 +31:39:25.9
68.47174 0.95316 galactic Cyg Second-epoch detections are separated by 0.8" and 8.8 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 | ASASSN-V J195951.08+313949.8 | 19:59:51.32 +31:39:49.8 (Gaia DR3) | SR (local) | 2458278.80360 (local) | Gaia3var=VARIABLE J-Ks=0.693+/-0.028 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:48.91 +31:39:25.9: 13.11 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:48.91 +31:39:25.9: 14.48 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J195951.08+313949.8,2461199.6702,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195951.08+313949.8 20260608.1702 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 06 08.1702 2461199.6702 12.12 19:58:16.39 +30:21:22.8
67.19060 0.55269 galactic Cyg Second-epoch detections are separated by 1.3" and 9.0 pix
The object was found in VSX 7" Gaia DR3 2030434454771275392
Type: E
# Max. Min./Amp. JD0 Period
18.770 G 19.190 G 0.839130000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:16.39 +30:21:22.8: 13.11 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:16.39 +30:21:22.8: 13.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030434454771275392,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030434454771275392 20260608.1702 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 06 08.1702 2461199.6702 12.33 19:58:41.31 +30:16:39.2
67.17036 0.43508 galactic Cyg Second-epoch detections are separated by 1.4" and 8.7 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 | 19:58:41.31 +30:16:39.2 (user input) | T | P | (position from user input) SpType: A2V (LAMOST DR5) J-Ks=0.165+/-0.033 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:41.31 +30:16:39.2: 13.42 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:41.31 +30:16:39.2: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.04 20:00:53.49 +30:40:33.3
67.75875 0.24068 galactic Cyg Second-epoch detections are separated by 0.4" and 8.8 pix
The object was found in VSX16" Gaia DR3 2030466615501280768
Type: L
# Max. Min./Amp. JD0 Period
17.530 G 17.790 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:53.49 +30:40:33.3: 13.12 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:53.49 +30:40:33.3: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030466615501280768,2461199.6702,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030466615501280768 20260608.1702 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 06 08.1702 2461199.6702 11.88 19:55:27.67 +26:03:33.3
63.19845 -1.15399 galactic Vul Second-epoch detections are separated by 0.7" and 8.9 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 | 19:55:27.67 +26:03:33.3 (user input) | T | P | (position from user input) J-Ks=1.024+/-0.041 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:55:27.67 +26:03:33.3: 12.67 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:55:27.67 +26:03:33.3: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.43 19:58:26.66 +29:33:48.2
66.53412 0.10638 galactic Cyg Second-epoch detections are separated by 0.5" and 8.8 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 J299.6138+29.5667 | 19:58:26.66 +29:33:48.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.240+/-0.033 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:26.66 +29:33:48.2: 13.43 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:26.66 +29:33:48.2: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.6138+29.5667,2461199.6702,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6138+29.5667 20260608.1702 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 06 08.1702 2461199.6702 11.73 19:57:43.61 +25:50:56.2
63.28329 -1.69842 galactic Vul Second-epoch detections are separated by 0.4" and 9.0 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 | ATO J299.4359+25.8488 | 19:57:43.53 +25:50:54.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.076+/-0.031 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:43.61 +25:50:56.2: 12.67 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:43.61 +25:50:56.2: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.4359+25.8488,2461199.6702,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.4359+25.8488 20260608.1702 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.79 19:59:00.74 +25:45:38.7
63.35925 -1.99121 galactic Vul Second-epoch detections are separated by 1.5" and 8.8 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 1835011346883316736 | 19:59:00.62 +25:45:39.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.838+/-0.027 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:00.74 +25:45:38.7: 12.66 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:00.74 +25:45:38.7: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1835011346883316736,2461199.6702,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1835011346883316736 20260608.1702 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.76 19:55:41.39 +25:46:53.7
62.98745 -1.34172 galactic Vul Second-epoch detections are separated by 1.1" and 9.0 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 | 19:55:41.39 +25:46:53.7 (user input) | T | P | (position from user input) J-Ks=0.239+/-0.034 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:55:41.39 +25:46:53.7: 12.66 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:55:41.39 +25:46:53.7: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.39 19:58:55.68 +29:48:04.0
66.79166 0.14136 galactic Cyg Second-epoch detections are separated by 1.7" and 8.6 pix
The object was found in VSX13" ZTF J195856.62+294808.0
Type: EW
# Max. Min./Amp. JD0 Period
20.507 r Y 0.481 r 2458367.69490 0.383651200000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:55.68 +29:48:04.0: 13.33 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:55.68 +29:48:04.0: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195856.62+294808.0,2461199.6702,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195856.62+294808.0 20260608.1702 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 06 08.1702 2461199.6702 12.35 20:01:21.70 +30:17:18.2
67.48318 -0.05000 galactic Cyg Second-epoch detections are separated by 0.7" and 9.0 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 | 20:01:21.70 +30:17:18.2 (user input) | T | P | (position from user input) J-Ks=0.760+/-0.028 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:21.70 +30:17:18.2: 13.27 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:21.70 +30:17:18.2: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.80 19:58:18.74 +30:34:52.9
67.38685 0.66314 galactic Cyg Second-epoch detections are separated by 1.6" and 9.0 pix
The object was found in VSX 1" Gaia DR3 2030453318314644992
Type: L
# Max. Min./Amp. JD0 Period
11.140 G 11.260 G M
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:18.74 +30:34:52.9: 12.68 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:18.74 +30:34:52.9: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030453318314644992,2461199.6702,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030453318314644992 20260608.1702 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 06 08.1702 2461199.6702 11.76 19:54:56.77 +26:13:02.2
63.27395 -0.97334 galactic Vul Second-epoch detections are separated by 0.6" and 8.9 pix
The object was found in VSX 1" ASASSN-V J195456.79+261302.6
Type: ROT
# Max. Min./Amp. JD0 Period
13.340 g Y 0.210 g 2458990.86900 0.858363000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:56.77 +26:13:02.2: 12.66 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:56.77 +26:13:02.2: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J195456.79+261302.6,2461199.6702,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195456.79+261302.6 20260608.1702 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 06 08.1702 2461199.6702 12.18 20:17:37.29 +26:53:19.4
66.56533 -4.89246 galactic Vul Second-epoch detections are separated by 2.0" and 9.1 pix
The object was found in VSX 2" CH Vul
Type: M
# Max. Min./Amp. JD0 Period
> 10.500 V < 14.300 V 2452855.00000 221.000000000000 M5
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:17:37.29 +26:53:19.4: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:17:37.29 +26:53:19.4: 13.18 +/- 0.03 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CH Vul,2461199.6702,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CH Vul 20260608.1702 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 06 08.1702 2461199.6702 12.18 19:59:25.11 +31:00:42.4
67.87795 0.68628 galactic Cyg Second-epoch detections are separated by 0.7" and 9.0 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 | ATO J299.8530+31.0153 | 19:59:25.11 +31:00:42.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.757+/-0.035 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:25.11 +31:00:42.4: 13.12 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:25.11 +31:00:42.4: 13.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.8530+31.0153,2461199.6702,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.8530+31.0153 20260608.1702 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 06 08.1702 2461199.6702 12.39 20:00:14.73 +31:15:57.2
68.18716 0.66930 galactic Cyg Second-epoch detections are separated by 0.7" and 8.8 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 J300.0684+31.2704 | 20:00:14.73 +31:15:57.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.287+/-0.059 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:14.73 +31:15:57.2: 13.44 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:14.73 +31:15:57.2: 14.27 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.0684+31.2704,2461199.6702,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0684+31.2704 20260608.1702 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 06 08.1702 2461199.6702 11.74 19:58:52.56 +30:10:44.2
67.10757 0.34893 galactic Cyg Second-epoch detections are separated by 0.6" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2030240867704428160 | 19:58:52.51 +30:10:44.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.742+/-0.028 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:52.56 +30:10:44.2: 12.66 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:52.56 +30:10:44.2: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030240867704428160,2461199.6702,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030240867704428160 20260608.1702 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.19 20:00:42.01 +31:22:50.4
68.33589 0.64724 galactic Cyg Second-epoch detections are separated by 1.7" and 9.1 pix
The object was found in VSX20" Gaia DR3 2030924184156069632
Type: ROT
# Max. Min./Amp. JD0 Period
16.310 G 16.350 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:42.01 +31:22:50.4: 13.07 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:42.01 +31:22:50.4: 14.49 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030924184156069632,2461199.6702,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030924184156069632 20260608.1702 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 06 08.1702 2461199.6702 12.16 20:00:26.60 +25:44:50.6
63.51701 -2.27254 galactic Vul Second-epoch detections are separated by 2.1" and 9.1 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 | 20:00:26.60 +25:44:50.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.361+/-0.030 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:26.60 +25:44:50.6: 13.11 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:26.60 +25:44:50.6: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.92 20:02:05.37 +33:25:18.5
70.22410 1.47680 galactic Cyg Second-epoch detections are separated by 1.2" and 8.8 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 J300.5306+33.4247 | 20:02:05.43 +33:25:18.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.648+/-0.027 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:05.37 +33:25:18.5: 12.92 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:05.37 +33:25:18.5: 14.79 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.5306+33.4247,2461199.6702,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.5306+33.4247 20260608.1702 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.94 19:57:31.57 +25:48:43.2
63.22821 -1.67913 galactic Vul Second-epoch detections are separated by 0.7" and 9.0 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 | 19:57:31.57 +25:48:43.2 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.223+/-0.030 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:31.57 +25:48:43.2: 12.91 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:31.57 +25:48:43.2: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.98 19:54:25.13 +26:04:08.8
63.08593 -0.94847 galactic Vul Second-epoch detections are separated by 1.7" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2026847946620449024 | 19:54:25.02 +26:03:28.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=11.937+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:25.13 +26:04:08.8: 12.91 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:25.13 +26:04:08.8: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2026847946620449024,2461199.6702,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026847946620449024 20260608.1702 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.04 19:59:18.72 +25:44:00.1
63.37126 -2.06304 galactic Vul Second-epoch detections are separated by 1.5" and 9.2 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 | 19:59:18.72 +25:44:00.1 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.032 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:18.72 +25:44:00.1: 12.92 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:18.72 +25:44:00.1: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.20 19:58:26.87 +29:45:35.7
66.70201 0.20855 galactic Cyg Second-epoch detections are separated by 3.8" and 9.4 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 | 19:58:26.87 +29:45:35.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:26.87 +29:45:35.7: 13.12 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:26.87 +29:45:35.7: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.02 19:59:42.53 +31:20:33.2
68.19209 0.80713 galactic Cyg Second-epoch detections are separated by 1.0" and 8.9 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 J299.9247+31.3433 | 19:59:42.53 +31:20:33.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.353+/-0.030 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:42.53 +31:20:33.2: 13.11 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:42.53 +31:20:33.2: 14.20 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.9247+31.3433,2461199.6702,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9247+31.3433 20260608.1702 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 06 08.1702 2461199.6702 12.20 20:00:52.30 +30:56:27.2
67.98159 0.38411 galactic Cyg Second-epoch detections are separated by 1.7" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.2299+30.9367 | 20:00:52.30 +30:56:27.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.446+/-0.027 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:52.30 +30:56:27.2: 13.42 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:52.30 +30:56:27.2: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.2299+30.9367,2461199.6702,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.2299+30.9367 20260608.1702 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 06 08.1702 2461199.6702 12.15 19:58:08.13 +30:28:25.7
67.27524 0.63939 galactic Cyg Second-epoch detections are separated by 1.5" and 9.0 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 | ATO J299.5239+30.4806 | 19:58:08.07 +30:28:24.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.069+/-0.025 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:08.13 +30:28:25.7: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:08.13 +30:28:25.7: 13.10 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.5239+30.4806,2461199.6702,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5239+30.4806 20260608.1702 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 06 08.1702 2461199.6702 12.18 19:57:22.56 +25:52:20.0
63.26203 -1.61893 galactic Vul Second-epoch detections are separated by 2.3" and 8.6 pix
The object was found in VSX 4" Gaia DR3 2026806272568030592
Type: L
# Max. Min./Amp. JD0 Period
17.820 G 18.070 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:22.56 +25:52:20.0: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:22.56 +25:52:20.0: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2026806272568030592,2461199.6702,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026806272568030592 20260608.1702 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 06 08.1702 2461199.6702 11.96 20:00:02.00 +30:43:22.7
67.70155 0.42227 galactic Cyg Second-epoch detections are separated by 0.2" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2030469192515681920 | 20:00:01.96 +30:43:22.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.758+/-0.026 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:02.00 +30:43:22.7: 12.90 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:02.00 +30:43:22.7: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2030469192515681920,2461199.6702,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2030469192515681920 20260608.1702 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 06 08.1702 2461199.6702 12.16 19:59:47.99 +29:47:38.9
66.88500 -0.02330 galactic Cyg Second-epoch detections are separated by 2.1" and 9.1 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 J299.9476+29.7947 | 19:59:48.03 +29:48:03.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.838+/-0.029 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:47.99 +29:47:38.9: 13.08 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:47.99 +29:47:38.9: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.9476+29.7947,2461199.6702,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9476+29.7947 20260608.1702 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 06 08.1702 2461199.6702 12.26 19:59:44.95 +31:22:27.4
68.22361 0.81647 galactic Cyg Second-epoch detections are separated by 5.0" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.9413+31.3679 | 19:59:44.95 +31:22:27.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.375+/-0.031 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:44.95 +31:22:27.4: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:44.95 +31:22:27.4: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.9413+31.3679,2461199.6702,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9413+31.3679 20260608.1702 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.26 19:59:47.63 +31:26:08.0
68.28076 0.84056 galactic Cyg Second-epoch detections are separated by 2.4" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.9393+31.4395 | 19:59:47.63 +31:26:08.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.311+/-0.030 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:47.63 +31:26:08.0: 13.11 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:47.63 +31:26:08.0: 14.56 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.9393+31.4395,2461199.6702,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9393+31.4395 20260608.1702 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.06 20:01:13.82 +32:18:50.8
69.18830 1.04417 galactic Cyg Second-epoch detections are separated by 0.7" and 8.8 pix
The object was found in VSX 0" Gaia DR3 2034083076732620672
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.870 G 12.970 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:13.82 +32:18:50.8: 13.08 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:13.82 +32:18:50.8: 15.61 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.08 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034083076732620672,2461199.6702,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2034083076732620672 20260608.1702 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 06 08.1702 2461199.6702 12.06 20:00:43.42 +30:58:10.9
67.98933 0.42626 galactic Cyg Second-epoch detections are separated by 0.3" and 9.0 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 | ATO J300.1744+30.9765 | 20:00:43.42 +30:58:10.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.271+/-0.036 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:43.42 +30:58:10.9: 13.09 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:43.42 +30:58:10.9: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.1744+30.9765,2461199.6702,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.1744+30.9765 20260608.1702 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 06 08.1702 2461199.6702 12.02 19:54:11.00 +25:56:29.2
62.94924 -0.96896 galactic Vul Second-epoch detections are separated by 3.6" and 8.5 pix
The object was found in VSX21" ZTF J195411.05+255608.3
Type: SR
# Max. Min./Amp. JD0 Period
19.094 r Y 0.165 r 2458588.85960 66.908131500000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:11.00 +25:56:29.2: 12.89 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:11.00 +25:56:29.2: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195411.05+255608.3,2461199.6702,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195411.05+255608.3 20260608.1702 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 06 08.1702 2461199.6702 12.11 19:57:27.14 +25:53:16.0
63.28426 -1.62548 galactic Vul Second-epoch detections are separated by 1.5" and 9.2 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 | 19:57:27.14 +25:53:16.0 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.031 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:27.14 +25:53:16.0: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:27.14 +25:53:16.0: 13.15 +/- 0.03 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.13 20:00:45.08 +30:10:54.7
67.32310 0.00570 galactic Cyg Second-epoch detections are separated by 1.5" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2030249152744337536 | 20:00:41.86 +30:10:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5III 1922ApJ....55...85L SA 64- 667 J-Ks=0.359+/-0.036 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:45.08 +30:10:54.7: 13.10 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:45.08 +30:10:54.7: 13.06 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030249152744337536,2461199.6702,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030249152744337536 20260608.1702 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 06 08.1702 2461199.6702 12.18 19:58:03.16 +29:31:38.0
66.45876 0.16008 galactic Cyg Second-epoch detections are separated by 1.2" and 8.8 pix
The object was found in VSX 1" Gaia DR3 2030109995793495424
Type: RS
# Max. Min./Amp. JD0 Period
12.770 G 12.830 G B
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:03.16 +29:31:38.0: 13.09 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:03.16 +29:31:38.0: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030109995793495424,2461199.6702,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030109995793495424 20260608.1702 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 06 08.1702 2461199.6702 11.77 19:58:03.83 +29:59:33.9
66.85697 0.40124 galactic Cyg Second-epoch detections are separated by 0.5" and 9.0 pix
The object was found in VSX 0" Gaia DR3 2030325878039959552
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.640 G 12.670 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:03.83 +29:59:33.9: 12.65 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:03.83 +29:59:33.9: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030325878039959552,2461199.6702,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030325878039959552 20260608.1702 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.75 19:58:51.92 +25:50:54.6
63.41675 -1.91710 galactic Vul Second-epoch detections are separated by 1.4" and 9.0 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 | ATO J299.7133+25.8453 | 19:58:51.84 +25:50:54.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.835+/-0.032 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:51.92 +25:50:54.6: 12.66 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:51.92 +25:50:54.6: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.7133+25.8453,2461199.6702,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.7133+25.8453 20260608.1702 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.19 20:02:33.38 +31:07:53.3
68.33429 0.17878 galactic Cyg Second-epoch detections are separated by 2.0" and 8.9 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 | Gaia DR3 2030878107744506112 | 20:02:31.05 +31:07:41.0 (Gaia DR3) | ROT (local) | (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.200+/-0.029 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:33.38 +31:07:53.3: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:33.38 +31:07:53.3: 14.90 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030878107744506112,2461199.6702,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030878107744506112 20260608.1702 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 06 08.1702 2461199.6702 12.22 19:57:55.49 +29:35:05.8
66.49346 0.21394 galactic Cyg Second-epoch detections are separated by 1.6" and 8.8 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 J299.4899+29.5761 | 19:57:55.49 +29:35:05.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.830+/-0.031 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:55.49 +29:35:05.8: 13.29 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:55.49 +29:35:05.8: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.4899+29.5761,2461199.6702,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.4899+29.5761 20260608.1702 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 06 08.1702 2461199.6702 12.14 19:59:17.68 +31:19:38.8
68.13279 0.87447 galactic Cyg Second-epoch detections are separated by 1.6" and 8.8 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 J299.8260+31.3298 | 19:59:20.76 +31:19:31.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.409+/-0.033 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:17.68 +31:19:38.8: 13.08 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:17.68 +31:19:38.8: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.8260+31.3298,2461199.6702,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.8260+31.3298 20260608.1702 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 06 08.1702 2461199.6702 12.11 19:55:19.04 +25:46:36.7
62.94000 -1.27241 galactic Vul Second-epoch detections are separated by 1.4" and 9.0 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 | 19:55:19.04 +25:46:36.7 (user input) | T | P | (position from user input) J-Ks=0.360+/-0.029 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:55:19.04 +25:46:36.7: 13.10 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:55:19.04 +25:46:36.7: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.75 19:56:28.94 +28:58:01.3
65.80214 0.16056 galactic Vul Second-epoch detections are separated by 0.2" and 8.9 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 | Gaia DR3 2028566831227030400 | 19:56:28.89 +28:58:00.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.644+/-0.032 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:28.94 +28:58:01.3: 12.64 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:28.94 +28:58:01.3: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2028566831227030400,2461199.6702,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2028566831227030400 20260608.1702 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.01 20:00:00.32 +31:15:01.3
68.14695 0.70478 galactic Cyg Second-epoch detections are separated by 0.7" and 8.9 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 | 20:00:00.32 +31:15:01.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:00.32 +31:15:01.3: 13.09 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:00.32 +31:15:01.3: 13.71 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.12 19:55:14.97 +26:04:55.4
63.19337 -1.10151 galactic Vul Second-epoch detections are separated by 4.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2026868150146608384 | 19:55:14.29 +26:04:33.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.984+/-0.030 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:55:14.97 +26:04:55.4: 13.04 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:55:14.97 +26:04:55.4: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2026868150146608384,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026868150146608384 20260608.1702 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 06 08.1702 2461199.6702 12.10 19:59:09.98 +29:43:59.5
66.76094 0.06171 galactic Cyg Second-epoch detections are separated by 0.7" and 8.9 pix
The object was found in VSX17" ZTF J195908.99+294410.8
Type: SR
# Max. Min./Amp. JD0 Period
18.676 r Y 0.133 r 2458428.64700 199.335301800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:09.98 +29:43:59.5: 13.07 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:09.98 +29:43:59.5: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195908.99+294410.8,2461199.6702,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195908.99+294410.8 20260608.1702 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 06 08.1702 2461199.6702 12.24 19:59:20.09 +30:31:40.8
67.45670 0.44768 galactic Cyg Second-epoch detections are separated by 3.0" and 8.8 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 J299.8443+30.5252 | 19:59:20.01 +30:31:40.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.579+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:20.09 +30:31:40.8: 13.26 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:20.09 +30:31:40.8: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.8443+30.5252,2461199.6702,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.8443+30.5252 20260608.1702 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.75 20:00:38.62 +25:58:43.6
63.73767 -2.18916 galactic Vul Second-epoch detections are separated by 0.7" and 8.9 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 | Gaia DR3 1835018596788389248 | 20:00:38.59 +25:58:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.242+/-0.032 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:38.62 +25:58:43.6: 12.65 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:38.62 +25:58:43.6: 12.71 +/- 0.02 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1835018596788389248,2461199.6702,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1835018596788389248 20260608.1702 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.02 20:01:04.18 +30:55:59.6
67.99749 0.34400 galactic Cyg Second-epoch detections are separated by 0.7" and 8.9 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 | Gaia DR3 2030848798893671552 | 20:01:01.45 +30:55:33.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.429+/-0.033 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:04.18 +30:55:59.6: 12.90 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:04.18 +30:55:59.6: 13.51 +/- 0.04 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030848798893671552,2461199.6702,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030848798893671552 20260608.1702 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 06 08.1702 2461199.6702 12.27 19:59:54.71 +31:15:44.6
68.14667 0.72810 galactic Cyg Second-epoch detections are separated by 0.7" and 9.0 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 | ATO J299.9695+31.2573 | 19:59:54.71 +31:15:44.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.727+/- (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:54.71 +31:15:44.6: 13.32 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:54.71 +31:15:44.6: 14.42 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.9695+31.2573,2461199.6702,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9695+31.2573 20260608.1702 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 06 08.1702 2461199.6702 11.93 20:02:46.86 +30:53:35.5
68.15794 0.01145 galactic Cyg Second-epoch detections are separated by 0.8" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.6959+30.8938 | 20:02:47.01 +30:53:37.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:46.86 +30:53:35.5: 12.89 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:46.86 +30:53:35.5: 13.44 +/- 0.04 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J300.6959+30.8938,2461199.6702,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.6959+30.8938 20260608.1702 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.94 19:59:09.04 +25:48:35.8
63.41750 -1.99199 galactic Vul Second-epoch detections are separated by 0.9" and 9.0 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 | ATO J299.7809+25.8057 | 19:59:08.99 +25:48:35.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.178+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:09.04 +25:48:35.8: 12.89 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:09.04 +25:48:35.8: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.7809+25.8057,2461199.6702,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.7809+25.8057 20260608.1702 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.91 20:00:36.60 +31:06:44.3
68.09767 0.52214 galactic Cyg Second-epoch detections are separated by 1.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.1478+31.1237 | 20:00:36.60 +31:06:44.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.239+/-0.030 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:36.60 +31:06:44.3: 12.86 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:36.60 +31:06:44.3: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.1478+31.1237,2461199.6702,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.1478+31.1237 20260608.1702 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.81 20:00:38.57 +25:46:05.9
63.55846 -2.29974 galactic Vul Second-epoch detections are separated by 0.2" and 9.0 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 | 20:00:38.57 +25:46:05.9 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.029 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:38.57 +25:46:05.9: 12.63 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:38.57 +25:46:05.9: 12.79 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.07 19:58:29.02 +29:52:12.4
66.79998 0.25958 galactic Cyg Second-epoch detections are separated by 1.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:58:29.02 +29:52:12.4 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.155+/-0.037 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:29.02 +29:52:12.4: 13.07 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:29.02 +29:52:12.4: 13.00 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.07 20:01:32.39 +30:38:28.9
67.80307 0.10404 galactic Cyg Second-epoch detections are separated by 0.4" and 8.9 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 J300.3861+30.6311 | 20:01:32.39 +30:38:28.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.334+/-0.028 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:32.39 +30:38:28.9: 13.08 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:32.39 +30:38:28.9: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.3861+30.6311,2461199.6702,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.3861+30.6311 20260608.1702 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.23 20:00:02.54 +30:01:23.4
67.10743 0.05245 galactic Cyg Second-epoch detections are separated by 1.4" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.0105+30.0267 | 20:00:02.54 +30:01:23.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.999+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:02.54 +30:01:23.4: 13.26 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:02.54 +30:01:23.4: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.0105+30.0267,2461199.6702,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0105+30.0267 20260608.1702 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 06 08.1702 2461199.6702 11.88 20:01:04.99 +30:23:00.4
67.53214 0.05124 galactic Cyg Second-epoch detections are separated by 0.6" and 8.9 pix
The object was found in VSX18" Gaia DR3 2030258636032915328
Type:
# Max. Min./Amp. JD0 Period
15.920 G 16.870 G B
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:04.99 +30:23:00.4: 12.87 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:04.99 +30:23:00.4: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030258636032915328,2461199.6702,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030258636032915328 20260608.1702 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.10 19:55:46.85 +28:46:00.4
65.55126 0.18791 galactic Vul Second-epoch detections are separated by 1.6" and 8.8 pix
The object was found in VSX 0" ZTF J195546.82+284600.2
Type: RS
# Max. Min./Amp. JD0 Period
13.114 r Y 0.018 r 2458605.94320 0.443183800000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:55:46.85 +28:46:00.4: 13.07 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:55:46.85 +28:46:00.4: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195546.82+284600.2,2461199.6702,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195546.82+284600.2 20260608.1702 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 06 08.1702 2461199.6702 12.10 19:58:01.29 +25:49:54.8
63.30332 -1.76389 galactic Vul Second-epoch detections are separated by 1.4" and 9.1 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 | 19:58:01.29 +25:49:54.8 (user input) | T | P | (position from user input) J-Ks=0.296+/-0.033 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:01.29 +25:49:54.8: 13.07 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:01.29 +25:49:54.8: 13.11 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.08 19:59:29.59 +30:57:40.2
67.84327 0.64609 galactic Cyg Second-epoch detections are separated by 0.5" and 8.8 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 | ASASSN-V J195931.13+305711.0 | 19:59:31.13 +30:57:11.0 (Gaia DR3) | SR (local) | 2459467.82000 (local) | Gaia3var=VARIABLE J-Ks=0.834+/-0.032 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:29.59 +30:57:40.2: 13.09 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:29.59 +30:57:40.2: 13.37 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195931.13+305711.0,2461199.6702,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195931.13+305711.0 20260608.1702 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.97 20:01:54.32 +30:45:43.8
67.94715 0.10132 galactic Cyg Second-epoch detections are separated by 1.9" and 8.8 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 2030655727185439360 | 20:01:54.30 +30:45:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.356+/-0.041 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:54.32 +30:45:43.8: 12.88 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:54.32 +30:45:43.8: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030655727185439360,2461199.6702,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030655727185439360 20260608.1702 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 06 08.1702 2461199.6702 11.93 20:00:48.54 +30:57:39.1
67.99147 0.40606 galactic Cyg Second-epoch detections are separated by 1.5" and 8.7 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 | 20:00:48.54 +30:57:39.1 (user input) | T | P | (position from user input) SpType: F3 (LAMOST DR5) J-Ks=0.241+/-0.028 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:48.54 +30:57:39.1: 12.86 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:48.54 +30:57:39.1: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.06 19:59:08.03 +30:19:59.8
67.26819 0.38242 galactic Cyg Second-epoch detections are separated by 1.6" and 8.9 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 | ZTF J195905.04+301951.8 | 19:59:06.25 +30:19:43.3 (Gaia DR3) | EA (local) | 2458292.96690 (local) | Gaia3var=NOT_AVAILABLE J-Ks=1.166+/-0.031 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:08.03 +30:19:59.8: 13.06 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:08.03 +30:19:59.8: 13.08 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195905.04+301951.8,2461199.6702,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195905.04+301951.8 20260608.1702 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 06 08.1702 2461199.6702 12.10 19:59:15.68 +30:48:16.4
67.68385 0.60624 galactic Cyg Second-epoch detections are separated by 0.8" and 8.9 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 | 19:59:15.68 +30:48:16.4 (user input) | T | P | (position from user input) J-Ks=11.328+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:15.68 +30:48:16.4: 13.08 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:15.68 +30:48:16.4: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.90 19:59:52.75 +31:07:20.5
68.02388 0.66043 galactic Cyg Second-epoch detections are separated by 0.3" and 8.9 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 J299.9748+31.1218 | 19:59:55.76 +31:07:33.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.339+/-0.030 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:52.75 +31:07:20.5: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:52.75 +31:07:20.5: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.9748+31.1218,2461199.6702,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9748+31.1218 20260608.1702 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.90 19:58:54.86 +30:15:50.5
67.18438 0.38646 galactic Cyg Second-epoch detections are separated by 1.9" and 8.8 pix
The object was found in VSX 2" ASASSN-V J195854.97+301548.6
Type: L:
# Max. Min./Amp. JD0 Period
13.150 V 13.270 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:54.86 +30:15:50.5: 12.87 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:54.86 +30:15:50.5: 12.84 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J195854.97+301548.6,2461199.6702,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195854.97+301548.6 20260608.1702 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.08 19:57:22.99 +29:38:30.4
66.48052 0.34403 galactic Cyg Second-epoch detections are separated by 0.4" and 8.9 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 | Gaia DR3 2030125801274177664 | 19:57:23.19 +29:39:09.7 (Gaia DR3) | E (local) | F (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.389+/-0.031 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:22.99 +29:38:30.4: 13.07 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:22.99 +29:38:30.4: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030125801274177664,2461199.6702,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030125801274177664 20260608.1702 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.68 19:59:07.95 +25:47:42.3
63.40269 -1.99629 galactic Vul Second-epoch detections are separated by 1.6" and 8.7 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 | ZTF J195905.49+254743.0 | 19:59:05.87 +25:48:06.6 (Gaia DR3) | RS (local) | 2458333.84140 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.748+/-0.029 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:07.95 +25:47:42.3: 12.62 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:07.95 +25:47:42.3: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195905.49+254743.0,2461199.6702,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195905.49+254743.0 20260608.1702 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.05 19:58:13.21 +25:48:33.1
63.30730 -1.81387 galactic Vul Second-epoch detections are separated by 1.2" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1834651840945246976 | 19:58:13.21 +25:48:33.1 (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=0.897+/-0.031 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:13.21 +25:48:33.1: 13.08 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:13.21 +25:48:33.1: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1834651840945246976,2461199.6702,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1834651840945246976 20260608.1702 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 06 08.1702 2461199.6702 12.22 19:55:17.20 +29:06:02.0
65.78078 0.45327 galactic Vul Second-epoch detections are separated by 3.0" and 9.4 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 | 19:55:17.20 +29:06:02.0 (user input) | T | P | (position from user input) J-Ks=0.396+/-0.031 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:55:17.20 +29:06:02.0: 13.08 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:55:17.20 +29:06:02.0: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.71 19:58:18.95 +29:58:29.4
66.87022 0.34535 galactic Cyg Second-epoch detections are separated by 0.7" and 8.8 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 | ASASSN-V J195819.62+295756.2 | 19:58:19.62 +29:57:56.2 (Gaia DR3) | SRS (local) | 2459153.73500 (local) | Gaia3var=NOT_AVAILABLE J-Ks=1.017+/-0.025 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:18.95 +29:58:29.4: 12.61 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:18.95 +29:58:29.4: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J195819.62+295756.2,2461199.6702,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195819.62+295756.2 20260608.1702 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.30 20:00:36.18 +30:14:19.7
67.35459 0.06296 galactic Cyg Second-epoch detections are separated by 2.8" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.1509+30.2362 | 20:00:36.18 +30:14:19.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.208+/-0.030 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:36.18 +30:14:19.7: 13.30 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:36.18 +30:14:19.7: 13.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.1509+30.2362,2461199.6702,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.1509+30.2362 20260608.1702 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 06 08.1702 2461199.6702 12.06 19:59:43.03 +31:55:48.6
68.69309 1.11430 galactic Cyg Second-epoch detections are separated by 2.5" and 9.2 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 | 19:59:43.03 +31:55:48.6 (user input) | T | P | (position from user input) J-Ks=0.288+/-0.032 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:43.03 +31:55:48.6: 13.09 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:43.03 +31:55:48.6: 15.69 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.09 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.85 19:59:59.29 +31:26:35.4
68.30903 0.80930 galactic Cyg Second-epoch detections are separated by 3.8" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.0102+31.4495 | 19:59:59.29 +31:26:35.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:59.29 +31:26:35.4: 12.85 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:59.29 +31:26:35.4: 13.70 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J300.0102+31.4495,2461199.6702,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0102+31.4495 20260608.1702 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 06 08.1702 2461199.6702 12.15 19:58:55.49 +30:52:15.4
67.70251 0.70255 galactic Cyg Second-epoch detections are separated by 0.2" and 8.8 pix
The object was found in VSX 1" Gaia DR3 2030487197019768064
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.940 G 12.990 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:55.49 +30:52:15.4: 13.06 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:55.49 +30:52:15.4: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030487197019768064,2461199.6702,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030487197019768064 20260608.1702 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 06 08.1702 2461199.6702 11.71 19:55:01.22 +25:49:31.5
62.94701 -1.19009 galactic Vul Second-epoch detections are separated by 1.2" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2026793181507108736 | 19:55:04.15 +25:49:22.5 (Gaia DR3) | ROT (local) | M (local) | Gaia3var=NOT_AVAILABLE J-Ks=1.023+/-0.033 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:55:01.22 +25:49:31.5: 12.59 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:55:01.22 +25:49:31.5: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2026793181507108736,2461199.6702,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026793181507108736 20260608.1702 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.70 20:01:08.51 +30:40:44.1
67.78972 0.19655 galactic Cyg Second-epoch detections are separated by 0.6" and 8.8 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 J300.2949+30.6856 | 20:01:08.52 +30:40:43.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.133+/-0.029 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:08.51 +30:40:44.1: 12.61 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:08.51 +30:40:44.1: 12.84 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.2949+30.6856,2461199.6702,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.2949+30.6856 20260608.1702 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.90 19:59:11.96 +29:58:34.4
66.97161 0.18309 galactic Cyg Second-epoch detections are separated by 0.7" and 8.8 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 J299.7980+29.9676 | 19:59:11.93 +29:58:34.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.843+/-0.031 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:11.96 +29:58:34.4: 12.83 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:11.96 +29:58:34.4: 12.87 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.7980+29.9676,2461199.6702,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.7980+29.9676 20260608.1702 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.09 19:57:39.70 +29:55:32.9
66.75439 0.44058 galactic Cyg Second-epoch detections are separated by 0.8" and 9.0 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 | ATO J299.4074+29.9226 | 19:57:39.70 +29:55:32.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.787+/-0.028 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:39.70 +29:55:32.9: 13.06 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:39.70 +29:55:32.9: 13.02 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.4074+29.9226,2461199.6702,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.4074+29.9226 20260608.1702 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 06 08.1702 2461199.6702 12.15 19:59:29.60 +32:27:20.2
69.11556 1.43045 galactic Cyg Second-epoch detections are separated by 1.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.8764+32.4543 | 19:59:29.60 +32:27:20.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.496+/-0.030 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:29.60 +32:27:20.2: 13.09 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:29.60 +32:27:20.2: 15.81 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.09 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.8764+32.4543,2461199.6702,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.8764+32.4543 20260608.1702 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 06 08.1702 2461199.6702 12.11 19:58:54.76 +30:13:37.9
67.15282 0.36747 galactic Cyg Second-epoch detections are separated by 0.9" and 8.7 pix
The object was found in VSX 1" ZTF J195854.66+301337.8
Type: RS
# Max. Min./Amp. JD0 Period
13.448 r Y 0.027 r 2458364.73710 0.601074300000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:54.76 +30:13:37.9: 13.06 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:54.76 +30:13:37.9: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195854.66+301337.8,2461199.6702,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195854.66+301337.8 20260608.1702 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 06 08.1702 2461199.6702 12.02 19:53:39.52 +25:49:37.7
62.79047 -0.92666 galactic Vul Second-epoch detections are separated by 1.1" and 9.0 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 | 19:53:39.52 +25:49:37.7 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.406+/-0.030 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:53:39.52 +25:49:37.7: 12.84 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:53:39.52 +25:49:37.7: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.95 19:57:49.48 +25:45:29.6
63.21732 -1.76451 galactic Vul Second-epoch detections are separated by 2.8" and 9.0 pix
The object was found in VSX24" Gaia DR3 1834649951159501696
Type: ROT
# Max. Min./Amp. JD0 Period
15.240 G 15.270 G 3.297860000000 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:49.48 +25:45:29.6: 13.06 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:49.48 +25:45:29.6: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1834649951159501696,2461199.6702,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834649951159501696 20260608.1702 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 06 08.1702 2461199.6702 11.69 20:00:34.10 +32:58:16.8
69.67333 1.50917 galactic Cyg Second-epoch detections are separated by 0.5" and 8.7 pix
The object was found in VSX 1" ASASSN-V J200034.08+325817.9
Type: SR
# Max. Min./Amp. JD0 Period
13.200 V 13.620 V 2458376.73450 65.612499300000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:34.10 +32:58:16.8: 13.02 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:34.10 +32:58:16.8: 15.42 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.02 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200034.08+325817.9,2461199.6702,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J200034.08+325817.9 20260608.1702 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.10 20:02:00.80 +30:45:35.1
67.95739 0.08036 galactic Cyg Second-epoch detections are separated by 0.2" and 8.9 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 J300.4928+30.7520 | 20:02:00.80 +30:45:35.1 (user input) | DBH (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.730+/-0.028 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:00.80 +30:45:35.1: 13.05 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:00.80 +30:45:35.1: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.4928+30.7520,2461199.6702,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.4928+30.7520 20260608.1702 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 06 08.1702 2461199.6702 12.28 19:59:42.83 +30:00:43.7
67.06066 0.10714 galactic Cyg Second-epoch detections are separated by 1.1" and 9.0 pix
The object was found in VSX 2" ZTF J195942.79+300045.5
Type: SR
# Max. Min./Amp. JD0 Period
13.075 r Y 0.069 r 2458332.75090 78.254532300000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:42.83 +30:00:43.7: 13.55 +/- 0.07 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:42.83 +30:00:43.7: 13.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195942.79+300045.5,2461199.6702,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195942.79+300045.5 20260608.1702 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.14 20:01:07.56 +29:35:24.2
66.86329 -0.37562 galactic Cyg Second-epoch detections are separated by 1.2" and 9.0 pix
The object was found in VSX 1" Gaia DR3 2030145867364994816
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.950 G 12.980 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:07.56 +29:35:24.2: 13.07 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:07.56 +29:35:24.2: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030145867364994816,2461199.6702,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030145867364994816 20260608.1702 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 06 08.1702 2461199.6702 12.30 19:58:45.69 +30:00:03.1
66.94290 0.27674 galactic Cyg Second-epoch detections are separated by 0.7" and 8.7 pix
The object was found in VSX 1" Gaia DR3 2030231354398265216
Type: ROT
# Max. Min./Amp. JD0 Period
13.100 G 13.140 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:45.69 +30:00:03.1: 13.40 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:45.69 +30:00:03.1: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030231354398265216,2461199.6702,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030231354398265216 20260608.1702 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 06 08.1702 2461199.6702 11.89 20:00:16.66 +30:31:25.4
67.55979 0.27270 galactic Cyg Second-epoch detections are separated by 0.8" and 8.8 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 2030276052076466048 | 20:00:16.65 +30:31:25.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.180+/-0.031 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:16.66 +30:31:25.4: 12.86 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:16.66 +30:31:25.4: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030276052076466048,2461199.6702,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030276052076466048 20260608.1702 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.25 19:56:45.22 +29:03:17.3
65.90796 0.15552 galactic Vul Second-epoch detections are separated by 1.5" and 9.0 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 | ATO J299.1935+29.0542 | 19:56:45.22 +29:03:17.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.389+/-0.036 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:45.22 +29:03:17.3: 13.24 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:45.22 +29:03:17.3: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.1935+29.0542,2461199.6702,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.1935+29.0542 20260608.1702 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 06 08.1702 2461199.6702 12.08 20:00:52.73 +29:45:24.0
66.97646 -0.24207 galactic Cyg Second-epoch detections are separated by 1.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.2192+29.7570 | 20:00:52.61 +29:45:25.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.390+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:52.73 +29:45:24.0: 12.98 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:52.73 +29:45:24.0: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.2192+29.7570,2461199.6702,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.2192+29.7570 20260608.1702 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.97 19:55:22.66 +28:43:22.7
65.46801 0.24080 galactic Vul Second-epoch detections are separated by 0.8" and 9.0 pix
The object was found in VSX 0" ASASSN-V J195522.64+284322.7
Type: EB
# Max. Min./Amp. JD0 Period
12.850 V 12.970 V 2457547.09700 1.328740000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:55:22.66 +28:43:22.7: 12.85 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:55:22.66 +28:43:22.7: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195522.64+284322.7,2461199.6702,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195522.64+284322.7 20260608.1702 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 06 08.1702 2461199.6702 11.87 19:53:54.89 +26:09:26.5
63.10325 -0.80604 galactic Vul Second-epoch detections are separated by 0.7" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2026864340527164416 | 19:53:54.70 +26:09:25.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:53:54.89 +26:09:26.5: 12.84 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:53:54.89 +26:09:26.5: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2026864340527164416,2461199.6702,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026864340527164416 20260608.1702 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.96 20:01:47.39 +31:27:57.3
68.53109 0.49490 galactic Cyg Second-epoch detections are separated by 1.0" and 8.7 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 2030901987739148672 | 20:01:47.39 +31:27:57.3 (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=0.263+/-0.031 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:47.39 +31:27:57.3: 12.83 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:47.39 +31:27:57.3: 15.81 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030901987739148672,2461199.6702,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2030901987739148672 20260608.1702 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 06 08.1702 2461199.6702 12.16 20:00:06.63 +31:57:06.3
68.75533 1.05466 galactic Cyg Second-epoch detections are separated by 0.8" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2033982441391864320 | 20:00:07.19 +31:56:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.230+/-0.031 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:06.63 +31:57:06.3: 13.04 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:06.63 +31:57:06.3: 15.75 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.04 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2033982441391864320,2461199.6702,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2033982441391864320 20260608.1702 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 06 08.1702 2461199.6702 12.09 19:57:24.87 +29:33:11.4
66.40845 0.29202 galactic Cyg Second-epoch detections are separated by 1.1" and 8.9 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 J299.3660+29.5560 | 19:57:24.87 +29:33:11.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.364+/-0.031 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:24.87 +29:33:11.4: 13.06 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:24.87 +29:33:11.4: 13.00 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.3660+29.5560,2461199.6702,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.3660+29.5560 20260608.1702 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 06 08.1702 2461199.6702 11.91 19:56:40.47 +28:47:29.5
65.67408 0.03339 galactic Vul Second-epoch detections are separated by 1.2" and 8.8 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 J299.1685+28.7945 | 19:56:40.44 +28:47:29.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.806+/-0.032 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:40.47 +28:47:29.5: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:40.47 +28:47:29.5: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.1685+28.7945,2461199.6702,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.1685+28.7945 20260608.1702 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.84 19:54:59.82 +25:50:47.0
62.96225 -1.17476 galactic Vul Second-epoch detections are separated by 1.7" and 8.9 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 | 19:54:59.82 +25:50:47.0 (user input) | T | P | (position from user input) J-Ks=0.443+/-0.042 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:59.82 +25:50:47.0: 12.83 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:59.82 +25:50:47.0: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.04 19:58:04.88 +29:55:30.9
66.80139 0.36274 galactic Cyg Second-epoch detections are separated by 1.1" and 9.0 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 | 19:58:04.88 +29:55:30.9 (user input) | T | P | (position from user input) J-Ks=0.633+/-0.029 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:04.88 +29:55:30.9: 13.04 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:04.88 +29:55:30.9: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.12 20:02:12.80 +30:37:53.8
67.87152 -0.02401 galactic Cyg Second-epoch detections are separated by 0.9" and 9.0 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 | ATO J300.5495+30.6307 | 20:02:12.80 +30:37:53.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.876+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:12.80 +30:37:53.8: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:12.80 +30:37:53.8: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.5495+30.6307,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.5495+30.6307 20260608.1702 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 06 08.1702 2461199.6702 11.36 19:54:15.51 +25:56:25.6
62.95709 -0.98395 galactic Vul Second-epoch detections are separated by 1.0" and 8.9 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 | Gaia DR3 2026844648085571712 | 19:54:15.38 +25:56:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:15.51 +25:56:25.6: 12.18 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:15.51 +25:56:25.6: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2026844648085571712,2461199.6702,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026844648085571712 20260608.1702 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.10 20:00:37.48 +30:55:34.7
67.94127 0.42142 galactic Cyg Second-epoch detections are separated by 1.7" and 9.0 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 | 20:00:37.48 +30:55:34.7 (user input) | T | P | (position from user input) J-Ks=0.193+/-0.030 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:37.48 +30:55:34.7: 13.05 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:37.48 +30:55:34.7: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.12 20:01:20.20 +31:12:16.0
68.25799 0.43873 galactic Cyg Second-epoch detections are separated by 1.1" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.3292+31.2016 | 20:01:20.20 +31:12:16.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.382+/-0.029 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:20.20 +31:12:16.0: 13.04 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:20.20 +31:12:16.0: 14.23 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.3292+31.2016,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.3292+31.2016 20260608.1702 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 06 08.1702 2461199.6702 11.73 19:56:58.18 +28:42:00.5
65.62969 -0.06940 galactic Vul Second-epoch detections are separated by 1.1" and 8.8 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 J299.2436+28.6976 | 19:56:58.24 +28:42:00.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.818+/-0.044 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:58.18 +28:42:00.5: 12.59 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:58.18 +28:42:00.5: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.2436+28.6976,2461199.6702,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.2436+28.6976 20260608.1702 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.24 20:00:28.39 +30:42:05.3
67.73304 0.33057 galactic Cyg Second-epoch detections are separated by 3.1" and 9.0 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 | ATO J300.1118+30.6981 | 20:00:28.39 +30:42:06.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.989+/-0.033 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:28.39 +30:42:05.3: 13.23 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:28.39 +30:42:05.3: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.1118+30.6981,2461199.6702,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.1118+30.6981 20260608.1702 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.00 20:00:34.21 +30:51:13.2
67.87337 0.39307 galactic Cyg Second-epoch detections are separated by 2.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.1469+30.8541 | 20:00:34.21 +30:51:13.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.287+/-0.028 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:34.21 +30:51:13.2: 13.04 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:34.21 +30:51:13.2: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.1469+30.8541,2461199.6702,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.1469+30.8541 20260608.1702 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 06 08.1702 2461199.6702 12.24 20:02:59.36 +30:19:08.0
67.69527 -0.33173 galactic Cyg Second-epoch detections are separated by 0.5" and 8.9 pix
The object was found in VSX11" Gaia DR3 2030580105725170688
Type: L
# Max. Min./Amp. JD0 Period
17.250 G 17.610 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:59.36 +30:19:08.0: 13.25 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:59.36 +30:19:08.0: 13.46 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030580105725170688,2461199.6702,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030580105725170688 20260608.1702 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.21 19:56:31.43 +28:46:24.2
65.64142 0.05217 galactic Vul Second-epoch detections are separated by 0.5" and 9.0 pix
The object was found in VSX 1" ZTF J195631.41+284623.7
Type: EW
# Max. Min./Amp. JD0 Period
12.916 r Y 0.320 r 2458356.79290 0.441564400000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:31.43 +28:46:24.2: 13.04 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:31.43 +28:46:24.2: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195631.41+284623.7,2461199.6702,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195631.41+284623.7 20260608.1702 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 06 08.1702 2461199.6702 12.18 19:56:42.55 +25:50:11.6
63.15350 -1.50935 galactic Vul Second-epoch detections are separated by 1.1" and 8.8 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 | 19:56:42.55 +25:50:11.6 (user input) | T | P | (position from user input) J-Ks=1.002+/-0.033 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:42.55 +25:50:11.6: 13.23 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:42.55 +25:50:11.6: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.19 19:58:40.90 +25:45:45.7
63.32194 -1.92674 galactic Vul Second-epoch detections are separated by 3.5" and 9.2 pix
The object was found in VSX18" Gaia DR3 1834647889575247872
Type: S
# Max. Min./Amp. JD0 Period
17.690 G 18.420 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:40.90 +25:45:45.7: 13.13 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:40.90 +25:45:45.7: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1834647889575247872,2461199.6702,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834647889575247872 20260608.1702 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 06 08.1702 2461199.6702 11.74 20:03:19.49 +25:51:04.5
63.94822 -2.76837 galactic Vul Second-epoch detections are separated by 3.1" and 8.6 pix
The object was found in VSX 1" NSVS 8409921
Type: SR
# Max. Min./Amp. JD0 Period
15.543 g Y 0.603 g 2458280.18860 130.667084200000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:03:19.49 +25:51:04.5: 12.58 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:03:19.49 +25:51:04.5: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 8409921,2461199.6702,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8409921 20260608.1702 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.62 19:57:19.44 +25:46:15.7
63.16951 -1.66162 galactic Vul Second-epoch detections are separated by 1.1" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2026798644706076800 | 19:57:19.38 +25:46:15.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.303+/-0.040 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:19.44 +25:46:15.7: 12.59 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:19.44 +25:46:15.7: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2026798644706076800,2461199.6702,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026798644706076800 20260608.1702 11.62CV 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 06 08.1702 2461199.6702 12.09 20:00:06.12 +30:58:39.6
67.92591 0.54373 galactic Cyg Second-epoch detections are separated by 1.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.0320+30.9622 | 20:00:08.38 +30:58:09.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A9V (LAMOST DR5) J-Ks=0.206+/-0.033 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:06.12 +30:58:39.6: 13.05 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:06.12 +30:58:39.6: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.0320+30.9622,2461199.6702,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.0320+30.9622 20260608.1702 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 06 08.1702 2461199.6702 11.65 19:54:46.74 +25:51:39.7
62.94945 -1.12520 galactic Vul Second-epoch detections are separated by 1.2" and 9.0 pix
The object was found in VSX15" Gaia DR3 2026840597947579648
Type: ROT
# Max. Min./Amp. JD0 Period
16.940 G 16.990 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:46.74 +25:51:39.7: 12.56 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:46.74 +25:51:39.7: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2026840597947579648,2461199.6702,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026840597947579648 20260608.1702 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.90 20:01:58.86 +30:15:36.8
67.53003 -0.17837 galactic Cyg Second-epoch detections are separated by 0.1" and 8.9 pix
The object was found in VSX21" Gaia DR3 2030207886695104512
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.360 G 14.410 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:58.86 +30:15:36.8: 12.81 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:58.86 +30:15:36.8: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030207886695104512,2461199.6702,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030207886695104512 20260608.1702 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.28 20:00:27.70 +26:07:33.7
63.84146 -2.07692 galactic Vul Second-epoch detections are separated by 2.7" and 9.4 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 | 20:00:27.70 +26:07:33.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.824+/-0.026 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:27.70 +26:07:33.7: 13.24 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:27.70 +26:07:33.7: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.65 19:57:42.15 +25:46:08.2
63.21213 -1.73545 galactic Vul Second-epoch detections are separated by 1.0" and 8.9 pix
The object was found in VSX18" Gaia DR3 1834650741433508224
Type: ROT
# Max. Min./Amp. JD0 Period
15.830 G 15.860 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:42.15 +25:46:08.2: 12.59 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:42.15 +25:46:08.2: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1834650741433508224,2461199.6702,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834650741433508224 20260608.1702 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.91 19:59:14.40 +25:59:16.8
63.57980 -1.91585 galactic Vul Second-epoch detections are separated by 0.6" and 8.9 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 J299.8065+25.9875 | 19:59:14.40 +25:59:16.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=10.585+/- (unrealisitic color!)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:14.40 +25:59:16.8: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:14.40 +25:59:16.8: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.8065+25.9875,2461199.6702,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.8065+25.9875 20260608.1702 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.66 19:54:32.43 +25:47:23.1
62.86068 -1.11602 galactic Vul Second-epoch detections are separated by 2.3" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2026833932158340992 | 19:54:32.41 +25:47:23.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.249+/-0.028 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:32.43 +25:47:23.1: 12.56 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:32.43 +25:47:23.1: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2026833932158340992,2461199.6702,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026833932158340992 20260608.1702 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.89 19:52:58.12 +26:12:11.1
63.03331 -0.60046 galactic Vul Second-epoch detections are separated by 0.7" and 9.1 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 | 19:52:58.12 +26:12:11.1 (user input) | T | P | (position from user input) J-Ks=0.624+/-0.027 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:52:58.12 +26:12:11.1: 12.81 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:52:58.12 +26:12:11.1: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.15 19:59:21.49 +29:43:58.4
66.78253 0.02609 galactic Cyg Second-epoch detections are separated by 1.5" and 9.1 pix
The object was found in VSX19" Gaia DR3 2030209840866672384
Type: ROT
# Max. Min./Amp. JD0 Period
14.910 G 14.940 G G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:21.49 +29:43:58.4: 13.04 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:21.49 +29:43:58.4: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030209840866672384,2461199.6702,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030209840866672384 20260608.1702 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 06 08.1702 2461199.6702 11.96 19:54:44.94 +28:49:21.6
65.48210 0.41027 galactic Vul Second-epoch detections are separated by 0.9" and 8.9 pix
The object was found in VSX14" Gaia DR3 2028560955711311872
Type: L
# Max. Min./Amp. JD0 Period
17.790 G 18.010 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:44.94 +28:49:21.6: 12.81 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:44.94 +28:49:21.6: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2028560955711311872,2461199.6702,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2028560955711311872 20260608.1702 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 06 08.1702 2461199.6702 12.16 19:58:19.56 +30:13:37.2
67.08631 0.47534 galactic Cyg Second-epoch detections are separated by 1.2" and 8.9 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 J299.5746+30.2246 | 19:58:19.56 +30:13:37.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.814+/-0.029 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:19.56 +30:13:37.2: 13.23 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:19.56 +30:13:37.2: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.5746+30.2246,2461199.6702,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5746+30.2246 20260608.1702 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 06 08.1702 2461199.6702 11.84 20:01:01.33 +31:30:17.6
68.47766 0.65443 galactic Cyg Second-epoch detections are separated by 0.8" and 9.0 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 | ATO J300.2553+31.5051 | 20:01:01.29 +31:30:18.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.406+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:01.33 +31:30:17.6: 12.80 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:01.33 +31:30:17.6: 14.82 +/- 0.14 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.2553+31.5051,2461199.6702,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.2553+31.5051 20260608.1702 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 06 08.1702 2461199.6702 11.31 19:59:36.56 +25:55:06.1
63.56400 -2.02305 galactic Vul Second-epoch detections are separated by 0.7" and 9.1 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 | ASASSN-V J195939.54+255458.7 | 19:59:39.54 +25:54:58.6 (Gaia DR3) | SR (local) | 527.000000000000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=1.210+/-0.032 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:36.56 +25:55:06.1: 12.15 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:36.56 +25:55:06.1: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J195939.54+255458.7,2461199.6702,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195939.54+255458.7 20260608.1702 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.18 19:58:07.93 +29:47:20.5
66.69101 0.28216 galactic Cyg Second-epoch detections are separated by 0.3" and 8.9 pix
The object was found in VSX13" Gaia DR3 2030131539351284608
Type: ROT
# Max. Min./Amp. JD0 Period
16.000 G 16.050 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:07.93 +29:47:20.5: 13.25 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:07.93 +29:47:20.5: 13.30 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030131539351284608,2461199.6702,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030131539351284608 20260608.1702 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 06 08.1702 2461199.6702 12.19 19:59:58.21 +30:58:22.3
67.90696 0.56524 galactic Cyg Second-epoch detections are separated by 1.8" and 9.1 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 J299.9923+30.9822 | 19:59:58.21 +30:58:22.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.201+/-0.033 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:58.21 +30:58:22.3: 13.23 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:58.21 +30:58:22.3: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.9923+30.9822,2461199.6702,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9923+30.9822 20260608.1702 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 06 08.1702 2461199.6702 12.12 19:59:04.74 +30:32:36.4
67.44095 0.50268 galactic Cyg Second-epoch detections are separated by 0.5" and 8.8 pix
The object was found in VSX14" Gaia DR3 2030461255378595200
Type: S
# Max. Min./Amp. JD0 Period
17.700 G 18.070 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:04.74 +30:32:36.4: 13.02 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:04.74 +30:32:36.4: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030461255378595200,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030461255378595200 20260608.1702 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 06 08.1702 2461199.6702 11.29 19:53:31.99 +26:01:32.9
62.94634 -0.80027 galactic Vul Second-epoch detections are separated by 1.1" and 8.9 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 | Gaia DR3 2026855853671795456 | 19:53:31.97 +26:01:32.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.495+/-0.038 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:53:31.99 +26:01:32.9: 12.14 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:53:31.99 +26:01:32.9: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2026855853671795456,2461199.6702,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026855853671795456 20260608.1702 11.29CV 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 06 08.1702 2461199.6702 12.23 20:02:06.14 +33:24:16.9
70.21100 1.46547 galactic Cyg Second-epoch detections are separated by 1.8" and 8.5 pix
The object was found in VSX 0" Gaia DR3 2058223374247698048
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.870 G 12.960 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:06.14 +33:24:16.9: 13.21 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:06.14 +33:24:16.9: 15.41 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.21 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2058223374247698048,2461199.6702,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2058223374247698048 20260608.1702 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 06 08.1702 2461199.6702 12.29 20:01:41.63 +31:00:41.3
68.13464 0.27179 galactic Cyg Second-epoch detections are separated by 1.3" and 8.8 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 | 20:01:41.63 +31:00:41.3 (user input) | T | P | (position from user input) J-Ks=0.741+/-0.026 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:41.63 +31:00:41.3: 13.22 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:41.63 +31:00:41.3: 14.76 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.62 20:00:35.11 +31:36:43.6
68.51966 0.79007 galactic Cyg Second-epoch detections are separated by 1.5" and 9.0 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 | ATO J300.1610+31.6132 | 20:00:35.08 +31:36:43.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.037+/-0.039 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:35.11 +31:36:43.6: 12.52 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:35.11 +31:36:43.6: 14.51 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.61 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J300.1610+31.6132,2461199.6702,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.1610+31.6132 20260608.1702 11.62CV 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 06 08.1702 2461199.6702 11.92 19:57:22.02 +29:19:28.2
66.20791 0.18165 galactic Vul Second-epoch detections are separated by 1.8" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.3362+29.3239 | 19:57:22.00 +29:19:35.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:22.02 +29:19:28.2: 12.80 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:22.02 +29:19:28.2: 12.90 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.86 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.3362+29.3239,2461199.6702,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.3362+29.3239 20260608.1702 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.12 19:58:15.88 +26:01:58.5
63.50342 -1.70558 galactic Vul Second-epoch detections are separated by 1.2" and 8.8 pix
The object was found in VSX11" Gaia DR3 2027183748657978368
Type: ROT
# Max. Min./Amp. JD0 Period
16.810 G 16.830 G 0.834310000000 F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:15.88 +26:01:58.5: 13.04 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:15.88 +26:01:58.5: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2027183748657978368,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2027183748657978368 20260608.1702 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 06 08.1702 2461199.6702 11.51 19:58:12.32 +25:57:27.2
63.43216 -1.73356 galactic Vul Second-epoch detections are separated by 2.5" and 8.9 pix
The object was found in VSX 1" ASASSN-V J195812.28+255728.4
Type: SRS
# Max. Min./Amp. JD0 Period
13.150 V 13.240 V 2457481.13200 20.059000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:12.32 +25:57:27.2: 12.53 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:12.32 +25:57:27.2: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J195812.28+255728.4,2461199.6702,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195812.28+255728.4 20260608.1702 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.11 19:58:25.41 +25:55:21.8
63.42807 -1.79358 galactic Vul Second-epoch detections are separated by 0.9" and 9.1 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 J299.6080+25.9229 | 19:58:25.41 +25:55:21.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.297+/-0.089 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:25.41 +25:55:21.8: 13.01 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:25.41 +25:55:21.8: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.6080+25.9229,2461199.6702,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6080+25.9229 20260608.1702 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 06 08.1702 2461199.6702 11.85 19:58:21.95 +29:55:36.4
66.83492 0.31099 galactic Cyg Second-epoch detections are separated by 4.5" and 8.9 pix
The object was found in VSX 4" Gaia DR3 2030136865110505984
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.900 G 12.930 G A
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:21.95 +29:55:36.4: 12.77 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:21.95 +29:55:36.4: 12.79 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030136865110505984,2461199.6702,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030136865110505984 20260608.1702 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 06 08.1702 2461199.6702 12.12 19:59:55.27 +30:06:35.9
67.16747 0.12041 galactic Cyg Second-epoch detections are separated by 1.7" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.9818+30.1117 | 19:59:55.27 +30:06:35.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.309+/-0.031 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:55.27 +30:06:35.9: 13.02 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:55.27 +30:06:35.9: 13.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.9818+30.1117,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9818+30.1117 20260608.1702 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 06 08.1702 2461199.6702 11.96 20:00:32.52 +30:48:48.7
67.83607 0.37705 galactic Cyg Second-epoch detections are separated by 1.4" and 8.7 pix
The object was found in VSX19" Gaia DR3 2030846462390112384
Type: L
# Max. Min./Amp. JD0 Period
18.050 G 18.390 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:32.52 +30:48:48.7: 13.02 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:32.52 +30:48:48.7: 13.17 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2030846462390112384,2461199.6702,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030846462390112384 20260608.1702 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 06 08.1702 2461199.6702 12.05 19:55:23.76 +26:11:07.0
63.29874 -1.07625 galactic Vul Second-epoch detections are separated by 1.9" and 8.9 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 J298.8374+26.1885 | 19:55:20.98 +26:11:18.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.752+/-0.032 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:55:23.76 +26:11:07.0: 13.03 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:55:23.76 +26:11:07.0: 13.17 +/- 0.03 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J298.8374+26.1885,2461199.6702,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.8374+26.1885 20260608.1702 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 06 08.1702 2461199.6702 11.65 19:54:35.82 +26:11:51.5
63.21668 -0.91641 galactic Vul Second-epoch detections are separated by 1.1" and 8.8 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 | 19:54:35.82 +26:11:51.5 (user input) | T | P | (position from user input) J-Ks=0.326+/-0.030 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:35.82 +26:11:51.5: 12.52 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:35.82 +26:11:51.5: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.29 20:02:36.32 +30:33:41.8
67.85694 -0.13266 galactic Cyg Second-epoch detections are separated by 0.5" and 8.9 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 | 20:02:36.32 +30:33:41.8 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.028 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:36.32 +30:33:41.8: 13.21 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:36.32 +30:33:41.8: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.34 20:05:58.29 +29:56:16.7
67.71790 -1.08031 galactic Cyg Second-epoch detections are separated by 2.6" and 9.0 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 | 20:05:58.29 +29:56:16.7 (user input) | T | P | (position from user input) J-Ks=0.895+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:05:58.29 +29:56:16.7: 13.19 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:05:58.29 +29:56:16.7: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.24 19:59:50.70 +25:46:43.8
63.47297 -2.14139 galactic Vul Second-epoch detections are separated by 2.6" and 9.4 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 | 19:59:50.70 +25:46:43.8 (user input) | T | P | (position from user input) J-Ks=0.452+/-0.030 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:50.70 +25:46:43.8: 13.23 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:50.70 +25:46:43.8: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.88 20:00:58.59 +30:35:14.3
67.69314 0.17838 galactic Cyg Second-epoch detections are separated by 0.5" and 8.8 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 J300.2341+30.5855 | 20:00:58.59 +30:35:14.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.221+/-0.029 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:58.59 +30:35:14.3: 12.79 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:58.59 +30:35:14.3: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.2341+30.5855,2461199.6702,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.2341+30.5855 20260608.1702 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.85 19:59:02.58 +32:05:07.0
68.75019 1.31734 galactic Cyg Second-epoch detections are separated by 0.4" and 8.8 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 J299.7687+32.0796 | 19:59:02.54 +32:05:06.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.762+/-0.027 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:02.58 +32:05:07.0: 12.79 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:02.58 +32:05:07.0: 15.96 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.79 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.7687+32.0796,2461199.6702,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.7687+32.0796 20260608.1702 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 06 08.1702 2461199.6702 11.85 19:57:21.70 +26:00:42.0
63.37945 -1.54357 galactic Vul Second-epoch detections are separated by 1.4" and 8.8 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 | 19:57:21.70 +26:00:42.0 (user input) | T | P | (position from user input) J-Ks=0.506+/-0.035 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:21.70 +26:00:42.0: 12.81 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:21.70 +26:00:42.0: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.65 20:01:06.84 +25:46:47.5
63.62419 -2.38384 galactic Vul Second-epoch detections are separated by 0.7" and 8.8 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 1834965476635143296 | 20:01:06.78 +25:46:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.917+/-0.027 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:06.84 +25:46:47.5: 12.52 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:06.84 +25:46:47.5: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1834965476635143296,2461199.6702,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834965476635143296 20260608.1702 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.09 19:57:08.50 +29:24:21.4
66.25185 0.26599 galactic Cyg Second-epoch detections are separated by 2.4" and 8.6 pix
The object was found in VSX16" Gaia DR3 2030084775744090496
Type: VAR
# Max. Min./Amp. JD0 Period
12.470 G 12.540 G 0.027783500000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:08.50 +29:24:21.4: 13.06 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:08.50 +29:24:21.4: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030084775744090496,2461199.6702,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030084775744090496 20260608.1702 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 06 08.1702 2461199.6702 12.07 19:57:44.32 +29:10:13.6
66.11876 0.03213 galactic Vul Second-epoch detections are separated by 1.4" and 9.1 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 J299.4339+29.1680 | 19:57:44.32 +29:10:13.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.383+/-0.044 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:44.32 +29:10:13.6: 13.05 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:44.32 +29:10:13.6: 13.19 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.4339+29.1680,2461199.6702,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.4339+29.1680 20260608.1702 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.05 19:58:38.60 +31:24:27.8
68.12832 1.03495 galactic Cyg Second-epoch detections are separated by 0.8" and 8.8 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 | 19:58:38.60 +31:24:27.8 (user input) | T | P | (position from user input) J-Ks=0.356+/-0.034 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:38.60 +31:24:27.8: 13.01 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:38.60 +31:24:27.8: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.01 19:58:52.11 +31:46:57.8
68.47300 1.19041 galactic Cyg Second-epoch detections are separated by 0.6" and 8.9 pix
The object was found in VSX 4" Gaia DR3 2033953785368046464
Type: L
# Max. Min./Amp. JD0 Period
17.980 G 18.270 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:52.11 +31:46:57.8: 12.96 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:52.11 +31:46:57.8: 15.48 +/- 0.28 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2033953785368046464,2461199.6702,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2033953785368046464 20260608.1702 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 06 08.1702 2461199.6702 12.44 19:57:38.81 +31:34:58.3
68.16672 1.30757 galactic Cyg Second-epoch detections are separated by 0.2" and 8.9 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 | 19:57:38.81 +31:34:58.3 (user input) | T | P | (position from user input) J-Ks=0.376+/-0.028 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:38.81 +31:34:58.3: 13.67 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:38.81 +31:34:58.3: 14.13 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.12 19:57:37.43 +25:51:03.0
63.27282 -1.67766 galactic Vul Second-epoch detections are separated by 3.0" and 8.7 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 | 19:57:37.43 +25:51:03.0 (user input) | T | P | (position from user input) J-Ks=0.993+/-0.033 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:37.43 +25:51:03.0: 13.21 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:37.43 +25:51:03.0: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.81 19:59:36.66 +30:48:43.4
67.72965 0.54627 galactic Cyg Second-epoch detections are separated by 1.4" and 9.0 pix
The object was found in VSX 2" ASASSN-V J195936.56+304844.2
Type: L
# Max. Min./Amp. JD0 Period
13.200 V 13.390 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:36.66 +30:48:43.4: 12.80 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:36.66 +30:48:43.4: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195936.56+304844.2,2461199.6702,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195936.56+304844.2 20260608.1702 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.11 19:55:53.90 +25:56:02.0
63.14207 -1.30294 galactic Vul Second-epoch detections are separated by 1.5" and 9.3 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 | ATO J298.9686+25.9324 | 19:55:53.81 +25:56:00.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.253+/-0.038 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:55:53.90 +25:56:02.0: 13.00 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:55:53.90 +25:56:02.0: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.9686+25.9324,2461199.6702,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J298.9686+25.9324 20260608.1702 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 06 08.1702 2461199.6702 11.84 20:00:38.18 +30:48:34.7
67.84345 0.35779 galactic Cyg Second-epoch detections are separated by 0.9" and 8.9 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 J300.1604+30.8172 | 20:00:38.18 +30:48:34.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.235+/-0.029 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:38.18 +30:48:34.7: 12.80 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:38.18 +30:48:34.7: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.1604+30.8172,2461199.6702,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.1604+30.8172 20260608.1702 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 06 08.1702 2461199.6702 11.96 19:57:18.37 +25:59:24.1
63.35447 -1.54419 galactic Vul Second-epoch detections are separated by 0.9" and 8.9 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 | 19:57:18.37 +25:59:24.1 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.031 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:18.37 +25:59:24.1: 12.79 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:18.37 +25:59:24.1: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.85 19:56:42.62 +29:35:47.2
66.36568 0.44527 galactic Cyg Second-epoch detections are separated by 1.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2030102638481543424 | 19:56:42.65 +29:35:47.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.778+/-0.032 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:42.62 +29:35:47.2: 12.79 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:42.62 +29:35:47.2: 12.86 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030102638481543424,2461199.6702,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030102638481543424 20260608.1702 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 06 08.1702 2461199.6702 12.17 19:59:09.14 +30:09:47.6
67.12549 0.28983 galactic Cyg Second-epoch detections are separated by 0.6" and 8.8 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 | 19:59:09.14 +30:09:47.6 (user input) | T | P | (position from user input) J-Ks=0.807+/-0.033 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:09.14 +30:09:47.6: 13.20 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:09.14 +30:09:47.6: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.94 20:02:53.01 +32:31:41.7
69.55477 0.86169 galactic Cyg Second-epoch detections are separated by 2.3" and 8.6 pix
The object was found in VSX 0" NSVS 8459011
Type: SR
# Max. Min./Amp. JD0 Period
14.889 g Y 0.685 g 2458341.45600 187.623593500000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:53.01 +32:31:41.7: 13.01 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:53.01 +32:31:41.7: 15.69 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.01 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 8459011,2461199.6702,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8459011 20260608.1702 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.98 19:54:32.12 +25:48:16.9
62.87289 -1.10731 galactic Vul Second-epoch detections are separated by 2.5" and 8.8 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 | 19:54:32.12 +25:48:16.9 (user input) | T | P | (position from user input) J-Ks=0.451+/-0.028 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:32.12 +25:48:16.9: 13.00 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:32.12 +25:48:16.9: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.12 20:00:05.10 +31:12:28.3
68.11976 0.66794 galactic Cyg Second-epoch detections are separated by 0.6" and 8.9 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 | Gaia DR3 2030915284983264768 | 20:00:05.08 +31:12:27.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.253+/-0.032 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:05.10 +31:12:28.3: 13.01 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:05.10 +31:12:28.3: 14.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030915284983264768,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030915284983264768 20260608.1702 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 06 08.1702 2461199.6702 11.97 20:00:46.53 +31:03:58.8
68.07729 0.46779 galactic Cyg Second-epoch detections are separated by 1.3" and 8.9 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 | 20:00:46.53 +31:03:58.8 (user input) | T | P | (position from user input) J-Ks=0.689+/-0.028 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:46.53 +31:03:58.8: 13.02 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:46.53 +31:03:58.8: 13.90 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.26 19:57:53.21 +29:28:32.3
66.39592 0.16391 galactic Cyg Second-epoch detections are separated by 1.2" and 9.1 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 | 19:57:53.21 +29:28:32.3 (user input) | T | P | (position from user input) J-Ks=0.683+/-0.032 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:53.21 +29:28:32.3: 13.20 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:53.21 +29:28:32.3: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.97 19:54:25.21 +26:03:29.8
63.07680 -0.95432 galactic Vul Second-epoch detections are separated by 3.0" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2026847946620449024 | 19:54:25.02 +26:03:28.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:25.21 +26:03:29.8: 13.00 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:25.21 +26:03:29.8: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2026847946620449024,2461199.6702,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026847946620449024 20260608.1702 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 06 08.1702 2461199.6702 12.11 20:01:45.36 +26:04:16.3
63.94811 -2.35277 galactic Vul Second-epoch detections are separated by 0.9" and 8.9 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 | 20:01:45.36 +26:04:16.3 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.028 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:45.36 +26:04:16.3: 13.01 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:45.36 +26:04:16.3: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.23 19:57:34.69 +29:08:13.4
66.07199 0.04461 galactic Vul Second-epoch detections are separated by 1.1" and 8.9 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 | 19:57:34.69 +29:08:13.4 (user input) | T | P | (position from user input) J-Ks=0.344+/-0.038 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:34.69 +29:08:13.4: 13.20 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:34.69 +29:08:13.4: 13.28 +/- 0.03 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.05 19:59:34.76 +29:55:24.1
66.96982 0.08528 galactic Cyg Second-epoch detections are separated by 0.6" and 8.9 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 J299.8971+29.9261 | 19:59:34.76 +29:55:24.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.340+/-0.032 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:34.76 +29:55:24.1: 12.98 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:34.76 +29:55:24.1: 13.09 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.8971+29.9261,2461199.6702,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.8971+29.9261 20260608.1702 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 06 08.1702 2461199.6702 11.98 19:59:49.89 +30:42:15.6
67.66288 0.44936 galactic Cyg Second-epoch detections are separated by 1.0" and 9.0 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 | ATO J299.9537+30.7045 | 19:59:49.89 +30:42:15.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.756+/-0.025 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:49.89 +30:42:15.6: 12.99 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:49.89 +30:42:15.6: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.9537+30.7045,2461199.6702,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9537+30.7045 20260608.1702 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.07 20:01:14.58 +26:09:44.5
63.96479 -2.20685 galactic Vul Second-epoch detections are separated by 1.3" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J300.3122+26.1630 | 20:01:13.22 +26:10:21.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.695+/-0.033 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:14.58 +26:09:44.5: 13.01 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:14.58 +26:09:44.5: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.3122+26.1630,2461199.6702,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.3122+26.1630 20260608.1702 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.08 19:57:04.06 +26:02:19.8
63.36827 -1.47303 galactic Vul Second-epoch detections are separated by 2.0" and 8.9 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 | 19:57:04.06 +26:02:19.8 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.323+/-0.030 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:04.06 +26:02:19.8: 12.98 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:04.06 +26:02:19.8: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.09 19:56:35.24 +28:47:50.4
65.66911 0.05273 galactic Vul Second-epoch detections are separated by 1.5" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2028516146285868288 | 19:56:35.22 +28:47:49.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.119+/-0.030 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:35.24 +28:47:50.4: 12.98 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:35.24 +28:47:50.4: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2028516146285868288,2461199.6702,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2028516146285868288 20260608.1702 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 06 08.1702 2461199.6702 11.90 19:58:23.69 +30:21:58.3
67.21273 0.53547 galactic Cyg Second-epoch detections are separated by 0.4" and 9.0 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 | Large-amplitude variable Gaia DR2 2030434660975291648 | 19:58:27.08 +30:21:47.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.247+/-0.041 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:23.69 +30:21:58.3: 12.78 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:23.69 +30:21:58.3: 12.78 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2030434660975291648,2461199.6702,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2030434660975291648 20260608.1702 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.84 20:02:01.27 +25:47:24.0
63.74067 -2.55195 galactic Vul Second-epoch detections are separated by 0.6" and 9.1 pix
The object was found in VSX15" Gaia DR3 1834976609165037312
Type: ROT
# Max. Min./Amp. JD0 Period
18.410 G 18.600 G 4.638610000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:01.27 +25:47:24.0: 12.77 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:01.27 +25:47:24.0: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1834976609165037312,2461199.6702,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834976609165037312 20260608.1702 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 06 08.1702 2461199.6702 11.65 20:00:12.46 +30:31:37.4
67.55469 0.28728 galactic Cyg Second-epoch detections are separated by 1.3" and 8.6 pix
The object was found in VSX 2" NSVS 8404238
Type: L
# Max. Min./Amp. JD0 Period
9.800 R1 10.650 R1
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:12.46 +30:31:37.4: 12.79 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:12.46 +30:31:37.4: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 8404238,2461199.6702,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8404238 20260608.1702 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.84 20:01:02.84 +30:43:29.0
67.81789 0.23799 galactic Cyg Second-epoch detections are separated by 0.3" and 8.9 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 J300.2617+30.7246 | 20:01:02.84 +30:43:29.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.243+/-0.026 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:02.84 +30:43:29.0: 12.77 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:02.84 +30:43:29.0: 13.07 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J300.2617+30.7246,2461199.6702,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.2617+30.7246 20260608.1702 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 06 08.1702 2461199.6702 12.38 19:56:40.48 +28:59:41.7
65.84783 0.13912 galactic Vul Second-epoch detections are separated by 1.9" and 8.7 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 | 19:56:40.48 +28:59:41.7 (user input) | T | P | (position from user input) J-Ks=0.715+/-0.030 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:40.48 +28:59:41.7: 13.51 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:40.48 +28:59:41.7: 13.46 +/- 0.03 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.04 19:57:47.19 +29:44:05.7
66.60568 0.31787 galactic Cyg Second-epoch detections are separated by 0.8" and 9.0 pix
The object was found in VSX 6" Gaia DR3 2030125045360142464
Type: L
# Max. Min./Amp. JD0 Period
16.860 G 17.310 G M
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:47.19 +29:44:05.7: 12.99 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:47.19 +29:44:05.7: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030125045360142464,2461199.6702,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030125045360142464 20260608.1702 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 06 08.1702 2461199.6702 12.29 19:56:48.33 +29:08:27.8
65.98751 0.19071 galactic Vul Second-epoch detections are separated by 2.3" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.2008+29.1411 | 19:56:48.33 +29:08:27.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.267+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:56:48.33 +29:08:27.8: 13.18 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:56:48.33 +29:08:27.8: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.2008+29.1411,2461199.6702,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.2008+29.1411 20260608.1702 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 06 08.1702 2461199.6702 12.07 19:54:34.17 +25:54:28.8
62.96536 -1.06060 galactic Vul Second-epoch detections are separated by 1.6" and 8.9 pix
The object was found in VSX23" Gaia DR3 2026841697459275904
Type: L
# Max. Min./Amp. JD0 Period
18.260 G 18.470 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:34.17 +25:54:28.8: 12.98 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:34.17 +25:54:28.8: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2026841697459275904,2461199.6702,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026841697459275904 20260608.1702 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.01 20:00:03.59 +32:07:43.1
68.90016 1.15682 galactic Cyg Second-epoch detections are separated by 1.7" and 8.8 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 | 20:00:03.59 +32:07:43.1 (user input) | T | P | (position from user input) J-Ks=0.351+/-0.028 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:03.59 +32:07:43.1: 12.98 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:03.59 +32:07:43.1: 15.87 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.98 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.08 19:59:36.70 +30:59:57.5
67.88907 0.64450 galactic Cyg Second-epoch detections are separated by 2.5" and 9.1 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 | ZTF J195932.89+310033.1 | 19:59:33.94 +31:00:21.0 (Gaia DR3) | SR (local) | 2458637.81460 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:36.70 +30:59:57.5: 12.98 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:36.70 +30:59:57.5: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195932.89+310033.1,2461199.6702,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195932.89+310033.1 20260608.1702 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.05 20:00:19.41 +31:21:48.0
68.27879 0.70644 galactic Cyg Second-epoch detections are separated by 1.6" and 9.1 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 | 20:00:19.41 +31:21:48.0 (user input) | T | P | (position from user input) J-Ks=0.803+/-0.030 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:19.41 +31:21:48.0: 12.98 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:19.41 +31:21:48.0: 14.17 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.97 19:58:09.81 +30:29:46.0
67.29741 0.64590 galactic Cyg Second-epoch detections are separated by 2.6" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:58:09.81 +30:29:46.0 (user input) | T | P | (position from user input) J-Ks=0.179+/-0.034 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:09.81 +30:29:46.0: 12.99 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:09.81 +30:29:46.0: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.10 19:58:46.52 +25:48:44.2
63.37526 -1.91879 galactic Vul Second-epoch detections are separated by 0.8" and 9.0 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 | ATO J299.6945+25.8141 | 19:58:46.52 +25:48:44.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.026+/-0.031 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:46.52 +25:48:44.2: 13.18 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:46.52 +25:48:44.2: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.6945+25.8141,2461199.6702,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6945+25.8141 20260608.1702 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 06 08.1702 2461199.6702 12.21 20:00:42.51 +30:25:21.0
67.52268 0.14047 galactic Cyg Second-epoch detections are separated by 1.6" and 9.1 pix
The object was found in VSX 8" NSV 12687
Type:
# Max. Min./Amp. JD0 Period
11.450 B B6
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:42.51 +30:25:21.0: 13.20 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:42.51 +30:25:21.0: 13.19 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 12687,2461199.6702,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 12687 20260608.1702 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 06 08.1702 2461199.6702 11.51 19:59:41.47 +31:57:21.6
68.71218 1.13256 galactic Cyg Second-epoch detections are separated by 0.5" and 8.8 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 J299.9214+31.9509 | 19:59:41.37 +31:57:21.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.026+/-0.027 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:41.47 +31:57:21.6: 12.48 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:41.47 +31:57:21.6: 15.59 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.48 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J299.9214+31.9509,2461199.6702,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.9214+31.9509 20260608.1702 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.96 20:00:58.16 +31:15:25.4
68.26119 0.53320 galactic Cyg Second-epoch detections are separated by 0.3" and 8.8 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 J300.2277+31.2581 | 20:00:58.16 +31:15:25.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.757+/-0.028 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:58.16 +31:15:25.4: 12.96 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:58.16 +31:15:25.4: 14.39 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J300.2277+31.2581,2461199.6702,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.2277+31.2581 20260608.1702 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 06 08.1702 2461199.6702 12.16 19:59:32.10 +30:29:14.3
67.44470 0.38962 galactic Cyg Second-epoch detections are separated by 1.5" and 9.0 pix
The object was found in VSX 1" ASASSN-V J195932.01+302914.5
Type: L
# Max. Min./Amp. JD0 Period
13.790 V 14.100 V
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:32.10 +30:29:14.3: 13.33 +/- 0.07 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:32.10 +30:29:14.3: 13.42 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195932.01+302914.5,2461199.6702,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195932.01+302914.5 20260608.1702 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 06 08.1702 2461199.6702 12.21 20:00:28.05 +31:32:04.9
68.44065 0.77058 galactic Cyg Second-epoch detections are separated by 1.4" and 8.9 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 | 20:00:28.05 +31:32:04.9 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.034 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:28.05 +31:32:04.9: 13.18 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:28.05 +31:32:04.9: 15.75 +/- 0.35 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.02 20:00:49.81 +30:19:15.9
67.45036 0.06468 galactic Cyg Second-epoch detections are separated by 0.7" and 8.8 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 J300.2076+30.3211 | 20:00:49.81 +30:19:15.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.239+/-0.033 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:49.81 +30:19:15.9: 12.98 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:49.81 +30:19:15.9: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.2076+30.3211,2461199.6702,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.2076+30.3211 20260608.1702 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 06 08.1702 2461199.6702 11.97 19:58:10.39 +25:52:58.3
63.36464 -1.76639 galactic Vul Second-epoch detections are separated by 1.3" and 9.2 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 | 19:58:10.39 +25:52:58.3 (user input) | T | P | (position from user input) J-Ks=0.837+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:10.39 +25:52:58.3: 12.98 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:10.39 +25:52:58.3: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.07 19:58:27.05 +29:56:32.1
66.85774 0.30339 galactic Cyg Second-epoch detections are separated by 1.3" and 9.1 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 J299.6126+29.9421 | 19:58:27.03 +29:56:31.6 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.323+/-0.053 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:27.05 +29:56:32.1: 12.98 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:27.05 +29:56:32.1: 12.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.6126+29.9421,2461199.6702,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6126+29.9421 20260608.1702 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.01 19:57:35.81 +29:13:08.8
66.14412 0.08393 galactic Vul Second-epoch detections are separated by 2.5" and 8.8 pix
The object was found in VSX15" ZTF J195734.71+291303.5
Type: SR
# Max. Min./Amp. JD0 Period
18.375 r Y 0.771 r 2458583.82070 147.422592900000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:35.81 +29:13:08.8: 12.98 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:35.81 +29:13:08.8: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195734.71+291303.5,2461199.6702,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J195734.71+291303.5 20260608.1702 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 06 08.1702 2461199.6702 11.92 19:57:53.05 +30:11:12.3
67.00211 0.53570 galactic Cyg Second-epoch detections are separated by 1.6" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2030425074607353984 | 19:57:50.73 +30:11:05.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.140+/-0.028 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:57:53.05 +30:11:12.3: 12.75 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:57:53.05 +30:11:12.3: 12.79 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2030425074607353984,2461199.6702,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2030425074607353984 20260608.1702 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.21 20:02:24.30 +30:19:20.6
67.63127 -0.22302 galactic Cyg Second-epoch detections are separated by 1.9" and 9.2 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 | 20:02:24.30 +30:19:20.6 (user input) | T | P | (position from user input) J-Ks=0.325+/-0.029 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:24.30 +30:19:20.6: 13.19 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:24.30 +30:19:20.6: 13.25 +/- 0.03 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 12.18 19:54:46.96 +28:52:19.0
65.52811 0.42941 galactic Vul Second-epoch detections are separated by 4.2" and 9.6 pix
The object was found in VSX12" Gaia DR3 2028573222138618112
Type: L
# Max. Min./Amp. JD0 Period
17.620 G 18.200 G
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:46.96 +28:52:19.0: 13.18 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:46.96 +28:52:19.0: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2028573222138618112,2461199.6702,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2028573222138618112 20260608.1702 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 06 08.1702 2461199.6702 11.74 19:59:36.34 +25:47:45.6
63.45931 -2.08652 galactic Vul Second-epoch detections are separated by 1.5" and 8.9 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 | 19:59:36.34 +25:47:45.6 (user input) | T | P | (position from user input) J-Ks=1.038+/-0.037 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:36.34 +25:47:45.6: 12.72 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:36.34 +25:47:45.6: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.81 19:54:07.40 +26:04:31.3
63.05707 -0.88839 galactic Vul Second-epoch detections are separated by 0.5" and 9.1 pix
The object was found in VSX 9" Gaia DR3 2026859873761081600
Type: ROT
# Max. Min./Amp. JD0 Period
14.520 G 14.560 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:54:07.40 +26:04:31.3: 12.75 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:54:07.40 +26:04:31.3: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2026859873761081600,2461199.6702,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2026859873761081600 20260608.1702 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.26 20:01:15.28 +30:37:51.6
67.76185 0.15063 galactic Cyg Second-epoch detections are separated by 2.1" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:01:15.28 +30:37:51.6 (user input) | T | P | (position from user input) J-Ks=0.444+/-0.033 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:01:15.28 +30:37:51.6: 13.16 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:01:15.28 +30:37:51.6: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.15 19:58:38.18 +26:03:11.1
63.56427 -1.76622 galactic Vul Second-epoch detections are separated by 1.5" and 9.3 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 | ATO J299.6563+26.0492 | 19:58:38.18 +26:03:11.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.844+/-0.028 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:38.18 +26:03:11.1: 13.19 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:38.18 +26:03:11.1: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.6563+26.0492,2461199.6702,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.6563+26.0492 20260608.1702 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 06 08.1702 2461199.6702 11.78 19:59:07.77 +31:19:42.1
68.11507 0.90498 galactic Cyg Second-epoch detections are separated by 0.9" and 9.0 pix
The object was found in VSX 1" Gaia DR3 2030932185640371712
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.520 G 12.550 G F
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:07.77 +31:19:42.1: 12.75 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:07.77 +31:19:42.1: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2030932185640371712,2461199.6702,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2030932185640371712 20260608.1702 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.12 19:58:22.47 +29:40:41.9
66.62412 0.17943 galactic Cyg Second-epoch detections are separated by 1.4" and 9.0 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 | ATO J299.5950+29.6811 | 19:58:22.47 +29:40:41.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.295+/-0.031 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:22.47 +29:40:41.9: 13.18 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:22.47 +29:40:41.9: 13.21 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.5950+29.6811,2461199.6702,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5950+29.6811 20260608.1702 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 06 08.1702 2461199.6702 12.24 20:02:30.99 +32:07:12.0
69.16762 0.71062 galactic Cyg Second-epoch detections are separated by 0.7" and 8.6 pix
The object was found in VSX17" Gaia DR3 2031067876576566016
Type: ROT
# Max. Min./Amp. JD0 Period
12.730 G 12.760 G K
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:30.99 +32:07:12.0: 13.08 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:30.99 +32:07:12.0: 15.79 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.08 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2031067876576566016,2461199.6702,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2031067876576566016 20260608.1702 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 11.52 19:58:00.42 +25:52:50.0
63.34316 -1.73571 galactic Vul Second-epoch detections are separated by 0.8" and 8.9 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 | Gaia DR3 1834653245365031424 | 19:58:00.42 +25:52:49.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.412+/-0.057 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:00.42 +25:52:50.0: 12.44 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:00.42 +25:52:50.0: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1834653245365031424,2461199.6702,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1834653245365031424 20260608.1702 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.27 20:02:24.13 +25:50:51.5
63.83503 -2.59424 galactic Vul Second-epoch detections are separated by 2.3" and 9.4 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 | 20:02:24.13 +25:50:51.5 (user input) | T | P | (position from user input) J-Ks=1.163+/-0.032 (M)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:02:24.13 +25:50:51.5: 13.34 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:02:24.13 +25:50:51.5: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.81 19:59:53.18 +30:24:20.5
67.41505 0.28231 galactic Cyg Second-epoch detections are separated by 0.3" and 8.8 pix
The object was found in VSX 0" V1023 Cyg
Type: EA/DM
# Max. Min./Amp. JD0 Period
12.800 pg 13.400 pg 2432797.39000 3.158817200000 A3:
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:53.18 +30:24:20.5: 13.16 +/- 0.05 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:53.18 +30:24:20.5: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1023 Cyg,2461199.6702,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1023 Cyg 20260608.1702 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1702 2461199.6702 12.20 20:00:24.59 +30:54:02.9
67.89531 0.44715 galactic Cyg Second-epoch detections are separated by 0.3" and 8.8 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 J300.1040+30.9046 | 20:00:24.59 +30:54:02.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.365+/-0.028 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 20:00:24.59 +30:54:02.9: 13.17 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 20:00:24.59 +30:54:02.9: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.1040+30.9046,2461199.6702,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J300.1040+30.9046 20260608.1702 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 06 08.1702 2461199.6702 12.34 19:58:02.07 +29:54:28.4
66.78129 0.36232 galactic Cyg Second-epoch detections are separated by 3.2" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J299.5097+29.9011 | 19:58:02.07 +29:54:28.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.368+/-0.029 (G)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:02.07 +29:54:28.4: 13.47 +/- 0.06 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:02.07 +29:54:28.4: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.5097+29.9011,2461199.6702,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J299.5097+29.9011 20260608.1702 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 06 08.1702 2461199.6702 11.96 19:58:46.45 +29:48:34.4
66.78137 0.17420 galactic Cyg Second-epoch detections are separated by 1.9" and 8.9 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 | Large-amplitude variable Gaia DR2 2030120612938278784 | 19:58:46.42 +29:48:35.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.806+/-0.032 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:46.45 +29:48:34.4: 12.93 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:46.45 +29:48:34.4: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2030120612938278784,2461199.6702,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2030120612938278784 20260608.1702 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 06 08.1702 2461199.6702 12.18 19:58:14.81 +26:04:09.8
63.53245 -1.68312 galactic Vul Second-epoch detections are separated by 2.3" and 8.8 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 | 19:58:14.81 +26:04:09.8 (user input) | T | P | (position from user input) J-Ks=0.616+/-0.031 (K)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:14.81 +26:04:09.8: 13.32 +/- 0.04 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:14.81 +26:04:09.8: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461199.6702,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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 06 08.1702 2461199.6702 11.85 19:59:01.92 +29:12:32.7
66.29934 -0.18823 galactic Vul Second-epoch detections are separated by 1.7" and 9.1 pix
The object was found in VSX 1" ASASSN-V J195901.90+291232.0
Type: SR
# Max. Min./Amp. JD0 Period
13.870 V 14.130 V 2457106.10000 221.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:59:01.92 +29:12:32.7: 12.72 +/- 0.02 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:59:01.92 +29:12:32.7: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J195901.90+291232.0,2461199.6702,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J195901.90+291232.0 20260608.1702 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 06 08.1702 2461199.6702 11.76 19:58:20.07 +25:51:00.4
63.35566 -1.81444 galactic Vul Second-epoch detections are separated by 1.4" and 8.8 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 | 19:58:20.07 +25:51:00.4 (user input) | T | P | (position from user input) J-Ks=0.280+/-0.031 (F)
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits at 19:58:20.07 +25:51:00.4: 12.73 +/- 0.03 detection
Forced photometry on wcs_Cyg-08-Q2b1x1_2026-05-17_05-22-14_20.00sec_-0.00C_LIGHT_1307.fits at 19:58:20.07 +25:51:00.4: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461199.6702,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260608.1702 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461153.93110167 23.04.2026 10:20:37.184 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits
First image: 2461153.93110167 23.04.2026 10:20:37.184 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits
Last image: 2461199.67048718 08.06.2026 04:05:20.092 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cyg-08-Q2b1x1_000732_TTUQ2b1x1_4080387_W1Z1EZvp/fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.66
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 22554
Objects passed selection criteria: 22515
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 15315.5
Average stars matched: 13000.5 (84.8846 %)
Memory usage VmPeak: 130776 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 00:14:22 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: 2461153.93110167 23.04.2026 10:20:37.184 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits
First image: 2461153.93110167 23.04.2026 10:20:37.184 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-08-Q2b1x1_2026-04-23_05-20-37_20.00sec_-4.90C_LIGHTs_0295.fits
Last image: 2461199.67048718 08.06.2026 04:05:20.092 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Cyg-08-Q2b1x1_000732_TTUQ2b1x1_4080387_W1Z1EZvp/fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 561
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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: 46 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 187438
Objects passed selection criteria: 186994
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: 128974
Average stars matched: 113585 (88.0683 %)
Memory usage VmPeak: 1967372 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 00:21:45 CDT 2026
Host name: tau
############################################################
**** FOUND 19:59:58.52 +31:27:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308118_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308118_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308124_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308124_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:54:06.18 +33:48:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 308125_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308125_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308126_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308126_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308130_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308130_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308257_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308257_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 20:01:21.91 +33:55:35.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308274_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308274_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:30:39.73 +27:54:36.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308297_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308297_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 20:03:50.43 +29:59:07.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308350_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308350_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308357_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308357_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308380_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308380_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:49:50.73 +28:27:42.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 308381_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308381_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 20:01:02.81 +27:43:55.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308406_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308406_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308410_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308410_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308438_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308438_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:54:21.80 +33:07:43.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308463_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 308463_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74154_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 74154_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90776_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 90776_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166332_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 166332_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20428_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 20428_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254792_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 254792_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:43.72 +30:49:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107567_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 107567_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104858_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 104858_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84847_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 84847_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112165_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 112165_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94508_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 94508_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134574_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 134574_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133570_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 133570_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131486_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 131486_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131622_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 131622_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124530_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 124530_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156272_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 156272_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76517_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 76517_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122125_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 122125_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140464_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 140464_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112575_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 112575_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99288_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 99288_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19980_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19980_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130420_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 130420_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 106638_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 106638_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 132451_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 132451_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 104691_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 104691_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 89892_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 89892_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 137338_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 137338_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 19179_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19179_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 75973_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 75973_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 162775_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 162775_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 104428_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 104428_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 123872_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 123872_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 118784_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 118784_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 121440_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 121440_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 140233_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 140233_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 137068_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 137068_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 150996_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 150996_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 22391_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 22391_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 81683_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 81683_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 88352_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 88352_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 134849_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 134849_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 83097_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 83097_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 117643_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 117643_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 93599_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 93599_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 21054_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21054_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 140859_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 140859_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 21015_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21015_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 123668_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 123668_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 28228_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 28228_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 152172_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 152172_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 121760_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 121760_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17630_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17630_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 119781_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 119781_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 113779_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 113779_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18393_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18393_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18586_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18586_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 100931_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 100931_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 20427_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 20427_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 253486_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 253486_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
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Considering the candidate 18568_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18568_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 110525_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 110525_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 20543_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 20543_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 114484_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 114484_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 26808_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 26808_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 26237_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 26237_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18460_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18460_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 20844_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 20844_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 235781_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 235781_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 19074_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19074_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 169958_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 169958_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 20119_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 20119_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 253243_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 253243_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
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Considering the candidate 17172_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17172_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17111_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17111_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 129099_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 129099_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 123218_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 123218_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 131214_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 131214_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 125426_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 125426_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 127823_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 127823_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 173202_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 173202_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 24555_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 24555_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 114300_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 114300_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 113641_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 113641_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18876_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18876_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 133425_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 133425_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 94558_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 94558_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 128574_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 128574_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 143681_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 143681_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 16664_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 16664_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 129262_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 129262_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 116979_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 116979_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 22041_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 22041_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:55:01.46 +26:04:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.426 2026870727126986496 298.75595749873 +26.06786797190 12.3999 11.2047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114815_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 114815_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18193_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18193_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 193601_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 193601_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 95758_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 95758_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18739_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18739_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 22307_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 22307_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 87408_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 87408_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 155898_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 155898_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 82745_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 82745_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18435_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18435_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 100982_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 100982_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18430_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18430_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 160136_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 160136_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 115039_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 115039_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18392_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18392_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 156074_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 156074_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:34.45 +31:42:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.836 2033951616370786048 299.64355189464 +31.71285127411 12.8194 12.4024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 158865_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 158865_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 20566_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 20566_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17631_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17631_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 146594_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 146594_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 111161_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 111161_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 132488_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 132488_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 171215_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 171215_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 145491_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 145491_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 25922_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 25922_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 21414_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21414_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 143786_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 143786_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 125699_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 125699_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 82092_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 82092_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 138421_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 138421_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 155285_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 155285_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 121073_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 121073_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 118964_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 118964_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 130506_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 130506_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 21977_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21977_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 99662_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 99662_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18838_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18838_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17662_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17662_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17263_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17263_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 106170_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 106170_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 120461_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 120461_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 127182_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 127182_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 24841_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 24841_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 113168_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 113168_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
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Considering the candidate 45720_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 45720_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 138599_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 138599_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 145293_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 145293_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 116637_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 116637_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 148783_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 148783_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17636_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17636_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 189848_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 189848_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17999_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17999_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 21924_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21924_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17011_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17011_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 105146_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 105146_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 147036_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 147036_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 137496_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 137496_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 124022_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 124022_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 19379_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19379_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 131339_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 131339_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 106476_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 106476_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 147910_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 147910_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 149556_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 149556_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 171349_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 171349_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 137957_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 137957_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 19624_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19624_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 19419_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19419_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 117226_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 117226_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 98699_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 98699_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 111354_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 111354_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 19105_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19105_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 142912_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 142912_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 100121_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 100121_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 146643_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 146643_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 16813_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 16813_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 84081_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 84081_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 144970_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 144970_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 22342_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 22342_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104516_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 104516_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126080_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 126080_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21974_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21974_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 137132_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 137132_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 145057_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 145057_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 137044_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 137044_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18496_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18496_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 141770_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 141770_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18221_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18221_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 108027_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 108027_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 129754_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 129754_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112922_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 112922_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122908_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 122908_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 78826_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 78826_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18535_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18535_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 137422_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 137422_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 133078_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 133078_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 137719_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 137719_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 120815_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 120815_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133158_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 133158_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 141587_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 141587_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103306_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 103306_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
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Considering the candidate 118915_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 118915_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 101414_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 101414_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18237_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18237_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18162_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18162_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 86909_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 86909_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 110954_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 110954_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 119022_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 119022_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 161756_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 161756_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 150105_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 150105_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 134706_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 134706_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17606_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17606_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 130588_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 130588_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 111233_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 111233_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 109202_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 109202_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 173977_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 173977_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 117785_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 117785_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17328_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17328_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17115_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17115_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 151383_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 151383_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:55.61 +31:30:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.178 2030940947373639808 299.98169560023 +31.50489624078 12.4176 11.4076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186331_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 186331_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 133063_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 133063_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 112314_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 112314_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 101489_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 101489_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 111611_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 111611_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 126400_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 126400_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 86248_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 86248_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 106009_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 106009_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 77623_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 77623_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 23555_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 23555_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 151207_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 151207_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 162405_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 162405_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 99114_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 99114_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 80110_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 80110_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18050_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18050_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 186533_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 186533_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:50:34.09 +32:54:45.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 109404_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 109404_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 129799_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 129799_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 19625_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19625_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 136822_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 136822_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 144468_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 144468_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 77786_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 77786_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 130916_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 130916_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 134913_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 134913_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 122017_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 122017_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 79235_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 79235_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18246_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18246_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17435_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17435_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 20641_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 20641_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17296_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17296_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 137886_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 137886_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 119463_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 119463_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:41.66 +30:17:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18278_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18278_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 119975_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 119975_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 24493_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 24493_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 17448_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17448_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 21677_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21677_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 16926_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 16926_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 24111_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 24111_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 104550_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 104550_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 79932_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 79932_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 127315_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 127315_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:39.96 +30:35:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117566_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 117566_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 151960_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 151960_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 20845_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 20845_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 105677_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 105677_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 137718_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 137718_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 126333_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 126333_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 21181_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21181_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 190051_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 190051_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 139417_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 139417_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 154449_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 154449_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 93343_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 93343_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 22390_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 22390_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234268_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 234268_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
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Considering the candidate 21230_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21230_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 188539_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 188539_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 20:01:48.27 +33:28:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 3.937 2058236293510389504 300.45035138386 +33.47963292296 9.0834 7.5597 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20312_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 20312_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 109782_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 109782_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115025_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 115025_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 133899_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 133899_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 24301_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 24301_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 24392_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 24392_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119232_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 119232_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
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Considering the candidate 128161_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 128161_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 113115_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 113115_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18025_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18025_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 128159_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 128159_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 165337_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 165337_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 21669_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21669_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18497_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18497_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 95668_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 95668_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 89586_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 89586_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 148528_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 148528_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 157936_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 157936_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 152451_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 152451_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18738_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18738_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 133616_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 133616_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 19845_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19845_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 133796_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 133796_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 21240_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21240_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 100019_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 100019_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 116148_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 116148_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 177213_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 177213_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17114_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 17114_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 143831_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 143831_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 140433_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 140433_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 97178_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 97178_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 21799_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21799_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 23930_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 23930_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 88562_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 88562_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 106756_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 106756_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
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Considering the candidate 109987_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 109987_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 130644_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 130644_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 25570_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 25570_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 21999_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 21999_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 80001_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 80001_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 121364_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 121364_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18949_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18949_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 126791_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 126791_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 131753_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 131753_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 84646_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 84646_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 103999_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 103999_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 88393_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 88393_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 19021_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19021_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 166612_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 166612_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 138300_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 138300_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 156269_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 156269_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:58:39.78 +31:42:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 0.601 2033951959968169472 299.66572380777 +31.71483457378 12.5278 12.0278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 147945_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 147945_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 124724_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 124724_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18345_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18345_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 123741_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 123741_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 94731_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 94731_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
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Considering the candidate 162488_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 162488_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 145454_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 145454_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 125049_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 125049_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 152354_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 152354_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 121169_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 121169_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 19491_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19491_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 110019_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 110019_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 151033_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 151033_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:59:57.47 +31:29:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.407 2030929200678183296 299.98935038505 +31.49021218217 11.8688 10.6427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90654_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 90654_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 116538_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 116538_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 121988_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 121988_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 84949_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
The candidate 84949_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091 did not pass the final checks
**** FOUND 19:55:03.32 +29:01:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81130_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 81130_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 18343_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 18343_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 22099_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 22099_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 129311_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 129311_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 22706_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 22706_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 146592_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 146592_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 102742_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 102742_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 167401_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 167401_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 19420_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19420_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 20072_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 20072_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 123017_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 123017_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 136130_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 136130_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 108882_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 108882_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 106351_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 106351_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 22885_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 22885_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 91148_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 91148_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
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Considering the candidate 19071_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
Preparing report for the candidate 19071_fd_Cyg-08-Q2b1x1_2026-06-07_23-05-20_20.00sec_4.90C_LIGHT_0091
make_report_in_HTML.sh Phase 2 (HTML assembly): 17s
make_report_in_HTML.sh TOTAL: 611s
Prepared the HTML report for the field Cyg-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:56:42.62 +29:35:47.2
19:57:55.49 +29:35:05.8
19:57:33.00 +29:37:15.8
19:59:07.44 +29:36:00.5
19:57:22.99 +29:38:30.4
20:01:07.56 +29:35:24.2
19:58:22.47 +29:40:41.9
19:57:47.19 +29:44:05.7
19:58:13.35 +29:44:38.5
19:59:09.98 +29:43:59.5
19:59:21.49 +29:43:58.4
19:59:02.01 +29:44:32.1
19:58:53.23 +29:45:03.1
19:58:26.87 +29:45:35.7
19:58:07.93 +29:47:20.5
20:00:52.73 +29:45:24.0
19:58:55.68 +29:48:04.0
19:58:46.45 +29:48:34.4
19:59:47.99 +29:47:38.9
19:59:43.57 +29:47:33.1
19:59:27.23 +29:50:21.7
19:58:29.02 +29:52:12.4
19:58:02.07 +29:54:28.4
19:57:39.70 +29:55:32.9
19:58:04.88 +29:55:30.9
19:58:21.95 +29:55:36.4
19:59:34.76 +29:55:24.1
19:58:27.05 +29:56:32.1
19:58:22.33 +29:57:37.3
19:58:18.95 +29:58:29.4
19:57:48.62 +29:59:35.9
19:59:11.96 +29:58:34.4
19:58:03.83 +29:59:33.9
19:58:45.69 +30:00:03.1
19:59:02.05 +30:00:13.6
19:59:42.83 +30:00:43.7
19:58:22.20 +30:02:32.2
20:00:02.54 +30:01:23.4
20:05:58.29 +29:56:16.7
19:58:21.53 +30:05:01.1
19:58:56.24 +30:04:00.0
20:03:09.52 +30:01:38.4
20:00:49.34 +30:03:56.3
19:59:35.27 +30:06:32.3
19:59:55.27 +30:06:35.9
19:58:26.78 +30:07:56.3
19:59:09.14 +30:09:47.6
19:57:53.05 +30:11:12.3
19:58:52.56 +30:10:44.2
19:59:22.85 +30:11:08.3
20:00:45.08 +30:10:54.7
19:58:19.56 +30:13:37.2
20:02:44.28 +30:09:48.8
19:58:54.76 +30:13:37.9
19:59:06.15 +30:15:35.4
19:58:54.86 +30:15:50.5
19:58:41.31 +30:16:39.2
20:00:36.18 +30:14:19.7
19:59:05.35 +30:17:17.9
20:01:58.86 +30:15:36.8
20:01:21.70 +30:17:18.2
19:59:08.03 +30:19:59.8
19:58:16.39 +30:21:22.8
20:00:49.81 +30:19:15.9
19:58:23.69 +30:21:58.3
20:01:30.96 +30:19:16.6
20:00:26.88 +30:20:56.8
20:02:24.30 +30:19:20.6
20:02:59.36 +30:19:08.0
19:58:49.33 +30:22:40.3
20:01:04.99 +30:23:00.4
19:59:53.18 +30:24:20.5
20:01:15.44 +30:23:20.1
20:00:15.48 +30:25:29.9
20:00:42.51 +30:25:21.0
19:58:08.89 +30:27:26.6
19:58:08.13 +30:28:25.7
20:00:06.26 +30:27:25.4
19:58:09.81 +30:29:46.0
19:59:32.10 +30:29:14.3
19:58:12.63 +30:30:42.9
20:01:05.47 +30:29:15.8
19:59:20.09 +30:31:40.8
19:59:04.74 +30:32:36.4
20:00:16.66 +30:31:25.4
20:00:12.46 +30:31:37.4
19:58:18.74 +30:34:52.9
20:02:07.55 +30:33:14.9
20:00:58.59 +30:35:14.3
20:02:36.32 +30:33:41.8
19:58:50.92 +30:38:18.2
20:00:48.41 +30:37:37.6
20:01:44.85 +30:36:59.9
20:01:15.28 +30:37:51.6
20:01:32.39 +30:38:28.9
20:02:12.80 +30:37:53.8
20:01:35.30 +30:39:54.5
20:00:53.49 +30:40:33.3
20:01:08.51 +30:40:44.1
19:59:49.89 +30:42:15.6
20:00:28.39 +30:42:05.3
19:59:02.39 +30:43:30.7
20:00:02.00 +30:43:22.7
19:59:55.88 +30:43:52.0
20:00:01.36 +30:43:57.1
20:01:02.84 +30:43:29.0
19:59:42.38 +30:46:18.0
19:59:03.28 +30:47:12.5
20:02:00.80 +30:45:35.1
20:01:54.32 +30:45:43.8
19:59:15.68 +30:48:16.4
20:00:09.95 +30:47:52.9
19:58:57.04 +30:49:27.2
19:59:36.66 +30:48:43.4
20:00:38.18 +30:48:34.7
20:00:32.52 +30:48:48.7
20:00:02.15 +30:51:15.2
19:58:55.49 +30:52:15.4
20:02:12.23 +30:49:33.0
20:00:34.21 +30:51:13.2
20:00:24.59 +30:54:02.9
20:00:37.48 +30:55:34.7
20:02:46.86 +30:53:35.5
19:59:31.13 +30:57:10.4
20:01:04.18 +30:55:59.6
20:00:12.42 +30:57:13.6
19:59:29.59 +30:57:40.2
20:00:52.30 +30:56:27.2
19:59:58.21 +30:58:22.3
20:00:48.54 +30:57:39.1
20:00:06.12 +30:58:39.6
20:00:43.42 +30:58:10.9
19:59:36.70 +30:59:57.5
19:59:33.89 +31:00:18.8
19:59:25.11 +31:00:42.4
20:01:41.63 +31:00:41.3
19:59:31.92 +31:04:18.6
20:00:46.53 +31:03:58.8
20:00:35.47 +31:04:10.7
20:01:36.08 +31:04:07.4
19:59:52.75 +31:07:20.5
20:00:36.60 +31:06:44.3
20:02:33.38 +31:07:53.3
19:59:55.54 +31:12:18.6
20:00:22.78 +31:12:04.9
20:00:05.10 +31:12:28.3
20:01:20.20 +31:12:16.0
20:00:00.32 +31:15:01.3
19:59:54.71 +31:15:44.6
20:00:14.73 +31:15:57.2
20:00:58.16 +31:15:25.4
20:00:55.43 +31:15:31.2
19:59:07.77 +31:19:42.1
19:59:20.79 +31:19:32.0
19:59:17.68 +31:19:38.8
19:59:42.53 +31:20:33.2
19:59:44.95 +31:22:27.4
20:00:19.41 +31:21:48.0
19:58:38.60 +31:24:27.8
20:00:42.01 +31:22:50.4
19:59:47.63 +31:26:08.0
19:59:59.29 +31:26:35.4
20:01:38.22 +31:27:49.9
20:01:47.39 +31:27:57.3
20:01:01.33 +31:30:17.6
20:00:13.59 +31:31:48.2
20:00:28.05 +31:32:04.9
19:57:38.81 +31:34:58.3
20:00:35.11 +31:36:43.6
19:59:48.91 +31:39:25.9
20:00:30.25 +31:40:36.0
20:00:07.21 +31:41:37.9
19:58:52.11 +31:46:57.8
20:00:35.55 +31:47:44.5
20:00:31.74 +31:51:06.3
19:59:43.03 +31:55:48.6
20:00:06.63 +31:57:06.3
19:59:41.47 +31:57:21.6
19:59:59.66 +31:58:05.8
19:59:02.58 +32:05:07.0
19:59:01.94 +32:07:51.9
20:00:03.59 +32:07:43.1
19:58:06.90 +25:43:31.1
20:02:30.99 +32:07:12.0
19:55:19.04 +25:46:36.7
19:54:32.43 +25:47:23.1
20:00:49.22 +32:15:28.5
19:59:18.72 +25:44:00.1
19:56:30.01 +25:46:24.1
19:54:32.12 +25:48:16.9
19:57:49.48 +25:45:29.6
20:00:13.73 +32:19:46.3
20:01:13.82 +32:18:50.8
19:57:41.93 +25:45:47.4
19:55:41.39 +25:46:53.7
19:57:19.44 +25:46:15.7
19:59:56.37 +32:24:56.1
19:53:39.52 +25:49:37.7
19:59:29.60 +32:27:20.2
19:58:40.90 +25:45:45.7
19:57:42.15 +25:46:08.2
19:55:01.22 +25:49:31.5
19:58:28.50 +25:46:25.3
19:59:21.96 +25:45:38.9
20:00:26.60 +25:44:50.6
19:59:00.74 +25:45:38.7
20:02:53.01 +32:31:41.7
19:57:31.57 +25:48:43.2
19:59:50.70 +25:46:43.8
19:54:59.82 +25:50:47.0
19:58:13.21 +25:48:33.1
20:00:15.72 +25:46:33.8
20:00:38.57 +25:46:05.9
19:59:07.95 +25:47:42.3
19:56:42.55 +25:50:11.6
19:54:46.74 +25:51:39.7
19:59:36.34 +25:47:45.6
19:58:46.52 +25:48:44.2
19:54:35.97 +25:52:08.6
19:57:52.09 +25:49:28.0
20:02:10.36 +25:45:33.1
20:01:44.93 +25:46:13.2
19:58:19.70 +25:49:11.5
19:59:09.04 +25:48:35.8
20:01:06.84 +25:46:47.5
19:58:01.29 +25:49:54.8
20:01:50.92 +25:46:33.9
19:54:59.59 +25:52:13.3
20:00:34.10 +32:58:16.8
19:57:37.43 +25:51:03.0
19:58:57.46 +25:49:51.1
19:57:43.61 +25:50:56.2
19:58:42.19 +25:50:16.2
20:02:01.27 +25:47:24.0
20:02:05.37 +33:25:18.5
20:02:06.14 +33:24:16.9
19:54:34.17 +25:54:28.8
19:58:20.07 +25:51:00.4
20:00:51.93 +25:49:06.9
19:58:51.92 +25:50:54.6
19:57:34.34 +25:52:41.3
20:01:44.41 +33:21:00.5
19:57:22.56 +25:52:20.0
19:57:27.14 +25:53:16.0
19:58:00.42 +25:52:50.0
19:58:10.39 +25:52:58.3
19:54:11.00 +25:56:29.2
19:54:15.51 +25:56:25.6
19:55:53.90 +25:56:02.0
19:57:39.51 +25:54:55.9
20:02:24.13 +25:50:51.5
19:58:45.81 +25:54:26.8
19:58:25.41 +25:55:21.8
20:01:17.30 +25:52:51.8
19:59:14.54 +25:54:46.8
20:02:05.32 +25:52:26.7
19:53:28.93 +25:57:40.5
20:03:19.49 +25:51:04.5
19:59:39.56 +25:55:00.5
19:59:36.56 +25:55:06.1
19:57:05.99 +25:58:00.7
20:02:18.84 +25:53:56.9
19:53:31.99 +26:01:32.9
19:58:12.32 +25:57:27.2
19:57:18.37 +25:59:24.1
19:57:49.50 +25:59:41.9
19:57:21.70 +26:00:42.0
19:59:14.40 +25:59:16.8
19:54:25.21 +26:03:29.8
19:54:25.13 +26:04:08.8
20:00:38.62 +25:58:43.6
19:55:27.67 +26:03:33.3
19:57:04.06 +26:02:19.8
19:54:07.40 +26:04:31.3
19:58:19.27 +26:01:55.4
19:55:14.97 +26:04:55.4
19:58:15.88 +26:01:58.5
20:00:57.01 +25:59:35.3
19:58:38.18 +26:03:11.1
19:58:14.81 +26:04:09.8
19:53:54.89 +26:09:26.5
20:01:56.56 +33:35:50.9
20:01:45.36 +26:04:16.3
19:52:58.12 +26:12:11.1
19:55:23.76 +26:11:07.0
19:54:35.82 +26:11:51.5
20:00:27.70 +26:07:33.7
19:54:49.28 +26:12:09.2
19:54:56.77 +26:13:02.2
20:01:14.58 +26:09:44.5
19:53:25.38 +26:18:02.4
20:01:41.88 +26:12:07.5
19:53:31.30 +26:20:57.6
19:53:33.24 +26:25:49.4
20:17:37.29 +26:53:19.4
19:55:42.18 +28:34:33.7
19:56:00.81 +28:38:25.8
19:56:12.07 +28:39:49.7
19:55:22.66 +28:43:22.7
19:56:58.18 +28:42:00.5
19:55:46.85 +28:46:00.4
19:56:31.43 +28:46:24.2
19:54:44.94 +28:49:21.6
19:56:35.24 +28:47:50.4
19:56:40.47 +28:47:29.5
19:54:46.96 +28:52:19.0
19:56:49.81 +28:52:07.3
19:57:29.34 +28:52:33.4
19:56:49.55 +28:54:45.5
19:57:14.83 +28:55:17.9
19:56:28.94 +28:58:01.3
19:56:40.48 +28:59:41.7
19:55:47.57 +29:00:54.1
19:56:45.22 +29:03:17.3
19:55:17.20 +29:06:02.0
19:56:31.44 +29:05:41.9
19:57:47.82 +29:07:01.6
19:56:48.33 +29:08:27.8
19:57:34.69 +29:08:13.4
19:57:44.32 +29:10:13.6
19:56:46.10 +29:12:02.6
19:57:35.81 +29:13:08.8
19:56:12.03 +29:14:46.0
19:59:01.92 +29:12:32.7
19:57:22.02 +29:19:28.2
20:00:16.53 +29:17:15.9
19:56:08.65 +29:23:24.3
19:58:14.32 +29:22:03.3
19:57:08.50 +29:24:21.4
19:57:12.81 +29:25:39.3
19:57:53.21 +29:28:32.3
19:58:03.16 +29:31:38.0
19:57:24.87 +29:33:11.4
19:57:27.51 +29:32:41.4
19:58:26.66 +29:33:48.2
########### Completed Cyg-08-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
19:55:42.18 +28:34:33.7
19:56:12.03 +29:14:46.0
19:59:01.94 +32:07:51.9
19:59:14.54 +25:54:46.8
19:59:27.23 +29:50:21.7
19:58:53.23 +29:45:03.1
19:55:47.57 +29:00:54.1
19:59:02.05 +30:00:13.6
19:56:08.65 +29:23:24.3
20:00:02.15 +30:51:15.2
19:58:57.04 +30:49:27.2
19:59:55.88 +30:43:52.0
20:00:01.36 +30:43:57.1
20:00:06.26 +30:27:25.4
20:00:07.21 +31:41:37.9
19:56:12.07 +28:39:49.7
19:58:49.33 +30:22:40.3
20:00:35.47 +31:04:10.7
19:58:22.20 +30:02:32.2
19:57:27.51 +29:32:41.4
19:57:39.51 +25:54:55.9
20:01:35.30 +30:39:54.5
19:59:43.57 +29:47:33.1
19:59:42.38 +30:46:18.0
19:59:02.01 +29:44:32.1
19:56:46.10 +29:12:02.6
20:00:12.42 +30:57:13.6
19:57:34.34 +25:52:41.3
19:56:00.81 +28:38:25.8
19:59:59.66 +31:58:05.8
19:58:13.35 +29:44:38.5
19:58:08.89 +30:27:26.6
19:59:06.15 +30:15:35.4
20:01:30.96 +30:19:16.6
19:59:31.92 +31:04:18.6
19:59:31.13 +30:57:10.4
20:01:38.22 +31:27:49.9
20:00:57.01 +25:59:35.3
19:56:49.81 +28:52:07.3
19:57:47.82 +29:07:01.6
20:02:12.23 +30:49:33.0
19:57:14.83 +28:55:17.9
20:02:44.28 +30:09:48.8
20:00:16.53 +29:17:15.9
20:02:18.84 +25:53:56.9
20:01:36.08 +31:04:07.4
19:57:05.99 +25:58:00.7
20:00:15.48 +30:25:29.9
19:53:33.24 +26:25:49.4
20:00:13.59 +31:31:48.2
20:00:26.88 +30:20:56.8
19:58:28.50 +25:46:25.3
19:59:05.35 +30:17:17.9
19:58:56.24 +30:04:00.0
19:57:52.09 +25:49:28.0
19:54:59.59 +25:52:13.3
19:57:33.00 +29:37:15.8
20:01:17.30 +25:52:51.8
20:01:50.92 +25:46:33.9
19:58:22.33 +29:57:37.3
20:02:05.32 +25:52:26.7
20:00:49.34 +30:03:56.3
19:53:31.30 +26:20:57.6
20:01:41.88 +26:12:07.5
19:58:19.70 +25:49:11.5
19:59:39.56 +25:55:00.5
20:01:56.56 +33:35:50.9
20:00:51.93 +25:49:06.9
20:00:49.22 +32:15:28.5
19:58:45.81 +25:54:26.8
19:57:41.93 +25:45:47.4
19:56:30.01 +25:46:24.1
20:00:48.41 +30:37:37.6
20:01:15.44 +30:23:20.1
19:59:02.39 +30:43:30.7
19:58:12.63 +30:30:42.9
20:02:07.55 +30:33:14.9
19:59:56.37 +32:24:56.1
19:54:49.28 +26:12:09.2
20:03:09.52 +30:01:38.4
19:58:21.53 +30:05:01.1
19:58:42.19 +25:50:16.2
20:00:09.95 +30:47:52.9
19:58:14.32 +29:22:03.3
19:58:50.92 +30:38:18.2
19:59:55.54 +31:12:18.6
19:58:06.90 +25:43:31.1
20:01:44.85 +30:36:59.9
19:59:22.85 +30:11:08.3
19:59:35.27 +30:06:32.3
20:00:15.72 +25:46:33.8
20:01:44.41 +33:21:00.5
19:57:12.81 +29:25:39.3
19:58:57.46 +25:49:51.1
19:58:19.27 +26:01:55.4
19:56:31.44 +29:05:41.9
20:00:30.25 +31:40:36.0
19:56:49.55 +28:54:45.5
20:01:44.93 +25:46:13.2
19:59:07.44 +29:36:00.5
20:02:10.36 +25:45:33.1
20:00:31.74 +31:51:06.3
19:58:26.78 +30:07:56.3
19:54:35.97 +25:52:08.6
20:00:35.55 +31:47:44.5
19:53:28.93 +25:57:40.5
19:59:21.96 +25:45:38.9
19:59:20.79 +31:19:32.0
19:57:48.62 +29:59:35.9
19:59:03.28 +30:47:12.5
20:00:13.73 +32:19:46.3
20:00:55.43 +31:15:31.2
19:53:25.38 +26:18:02.4
19:57:49.50 +25:59:41.9
20:00:22.78 +31:12:04.9
20:01:05.47 +30:29:15.8
19:57:29.34 +28:52:33.4
19:59:33.89 +31:00:18.8
19:59:48.91 +31:39:25.9
19:58:16.39 +30:21:22.8
19:58:41.31 +30:16:39.2
20:00:53.49 +30:40:33.3
19:55:27.67 +26:03:33.3
19:58:26.66 +29:33:48.2
19:57:43.61 +25:50:56.2
19:59:00.74 +25:45:38.7
19:55:41.39 +25:46:53.7
19:58:55.68 +29:48:04.0
20:01:21.70 +30:17:18.2
19:58:18.74 +30:34:52.9
19:54:56.77 +26:13:02.2
20:17:37.29 +26:53:19.4
19:59:25.11 +31:00:42.4
20:00:14.73 +31:15:57.2
19:58:52.56 +30:10:44.2
20:00:42.01 +31:22:50.4
20:00:26.60 +25:44:50.6
20:02:05.37 +33:25:18.5
19:57:31.57 +25:48:43.2
19:54:25.13 +26:04:08.8
19:59:18.72 +25:44:00.1
19:58:26.87 +29:45:35.7
19:59:42.53 +31:20:33.2
20:00:52.30 +30:56:27.2
19:58:08.13 +30:28:25.7
19:57:22.56 +25:52:20.0
20:00:02.00 +30:43:22.7
19:59:47.99 +29:47:38.9
19:59:44.95 +31:22:27.4
19:59:47.63 +31:26:08.0
20:01:13.82 +32:18:50.8
20:00:43.42 +30:58:10.9
19:54:11.00 +25:56:29.2
19:57:27.14 +25:53:16.0
20:00:45.08 +30:10:54.7
19:58:03.16 +29:31:38.0
19:58:03.83 +29:59:33.9
19:58:51.92 +25:50:54.6
20:02:33.38 +31:07:53.3
19:57:55.49 +29:35:05.8
19:59:17.68 +31:19:38.8
19:55:19.04 +25:46:36.7
19:56:28.94 +28:58:01.3
20:00:00.32 +31:15:01.3
19:55:14.97 +26:04:55.4
19:59:09.98 +29:43:59.5
19:59:20.09 +30:31:40.8
20:00:38.62 +25:58:43.6
20:01:04.18 +30:55:59.6
19:59:54.71 +31:15:44.6
20:02:46.86 +30:53:35.5
19:59:09.04 +25:48:35.8
20:00:36.60 +31:06:44.3
20:00:38.57 +25:46:05.9
19:58:29.02 +29:52:12.4
20:01:32.39 +30:38:28.9
20:00:02.54 +30:01:23.4
20:01:04.99 +30:23:00.4
19:55:46.85 +28:46:00.4
19:58:01.29 +25:49:54.8
19:59:29.59 +30:57:40.2
20:01:54.32 +30:45:43.8
20:00:48.54 +30:57:39.1
19:59:08.03 +30:19:59.8
19:59:15.68 +30:48:16.4
19:59:52.75 +31:07:20.5
19:58:54.86 +30:15:50.5
19:57:22.99 +29:38:30.4
19:59:07.95 +25:47:42.3
19:58:13.21 +25:48:33.1
19:55:17.20 +29:06:02.0
19:58:18.95 +29:58:29.4
20:00:36.18 +30:14:19.7
19:59:43.03 +31:55:48.6
19:59:59.29 +31:26:35.4
19:58:55.49 +30:52:15.4
19:55:01.22 +25:49:31.5
20:01:08.51 +30:40:44.1
19:59:11.96 +29:58:34.4
19:57:39.70 +29:55:32.9
19:59:29.60 +32:27:20.2
19:58:54.76 +30:13:37.9
19:53:39.52 +25:49:37.7
19:57:49.48 +25:45:29.6
20:00:34.10 +32:58:16.8
20:02:00.80 +30:45:35.1
19:59:42.83 +30:00:43.7
20:01:07.56 +29:35:24.2
19:58:45.69 +30:00:03.1
20:00:16.66 +30:31:25.4
19:56:45.22 +29:03:17.3
20:00:52.73 +29:45:24.0
19:55:22.66 +28:43:22.7
19:53:54.89 +26:09:26.5
20:01:47.39 +31:27:57.3
20:00:06.63 +31:57:06.3
19:57:24.87 +29:33:11.4
19:56:40.47 +28:47:29.5
19:54:59.82 +25:50:47.0
19:58:04.88 +29:55:30.9
20:02:12.80 +30:37:53.8
19:54:15.51 +25:56:25.6
20:00:37.48 +30:55:34.7
20:01:20.20 +31:12:16.0
19:56:58.18 +28:42:00.5
20:00:28.39 +30:42:05.3
20:00:34.21 +30:51:13.2
20:02:59.36 +30:19:08.0
19:56:31.43 +28:46:24.2
19:56:42.55 +25:50:11.6
19:58:40.90 +25:45:45.7
20:03:19.49 +25:51:04.5
19:57:19.44 +25:46:15.7
20:00:06.12 +30:58:39.6
19:54:46.74 +25:51:39.7
20:01:58.86 +30:15:36.8
20:00:27.70 +26:07:33.7
19:57:42.15 +25:46:08.2
19:59:14.40 +25:59:16.8
19:54:32.43 +25:47:23.1
19:52:58.12 +26:12:11.1
19:59:21.49 +29:43:58.4
19:54:44.94 +28:49:21.6
19:58:19.56 +30:13:37.2
20:01:01.33 +31:30:17.6
19:59:36.56 +25:55:06.1
19:58:07.93 +29:47:20.5
19:59:58.21 +30:58:22.3
19:59:04.74 +30:32:36.4
19:53:31.99 +26:01:32.9
20:02:06.14 +33:24:16.9
20:01:41.63 +31:00:41.3
20:00:35.11 +31:36:43.6
19:57:22.02 +29:19:28.2
19:58:15.88 +26:01:58.5
19:58:12.32 +25:57:27.2
19:58:25.41 +25:55:21.8
19:58:21.95 +29:55:36.4
19:59:55.27 +30:06:35.9
20:00:32.52 +30:48:48.7
19:55:23.76 +26:11:07.0
19:54:35.82 +26:11:51.5
20:02:36.32 +30:33:41.8
20:05:58.29 +29:56:16.7
19:59:50.70 +25:46:43.8
20:00:58.59 +30:35:14.3
19:59:02.58 +32:05:07.0
19:57:21.70 +26:00:42.0
20:01:06.84 +25:46:47.5
19:57:08.50 +29:24:21.4
19:57:44.32 +29:10:13.6
19:58:38.60 +31:24:27.8
19:58:52.11 +31:46:57.8
19:57:38.81 +31:34:58.3
19:57:37.43 +25:51:03.0
19:59:36.66 +30:48:43.4
19:55:53.90 +25:56:02.0
20:00:38.18 +30:48:34.7
19:57:18.37 +25:59:24.1
19:56:42.62 +29:35:47.2
19:59:09.14 +30:09:47.6
20:02:53.01 +32:31:41.7
19:54:32.12 +25:48:16.9
20:00:05.10 +31:12:28.3
20:00:46.53 +31:03:58.8
19:57:53.21 +29:28:32.3
19:54:25.21 +26:03:29.8
20:01:45.36 +26:04:16.3
19:57:34.69 +29:08:13.4
19:59:34.76 +29:55:24.1
19:59:49.89 +30:42:15.6
20:01:14.58 +26:09:44.5
19:57:04.06 +26:02:19.8
19:56:35.24 +28:47:50.4
19:58:23.69 +30:21:58.3
20:02:01.27 +25:47:24.0
20:00:12.46 +30:31:37.4
20:01:02.84 +30:43:29.0
19:56:40.48 +28:59:41.7
19:57:47.19 +29:44:05.7
19:56:48.33 +29:08:27.8
19:54:34.17 +25:54:28.8
20:00:03.59 +32:07:43.1
19:59:36.70 +30:59:57.5
20:00:19.41 +31:21:48.0
19:58:09.81 +30:29:46.0
19:58:46.52 +25:48:44.2
20:00:42.51 +30:25:21.0
19:59:41.47 +31:57:21.6
20:00:58.16 +31:15:25.4
19:59:32.10 +30:29:14.3
20:00:28.05 +31:32:04.9
20:00:49.81 +30:19:15.9
19:58:10.39 +25:52:58.3
19:58:27.05 +29:56:32.1
19:57:35.81 +29:13:08.8
19:57:53.05 +30:11:12.3
20:02:24.30 +30:19:20.6
19:54:46.96 +28:52:19.0
19:59:36.34 +25:47:45.6
19:54:07.40 +26:04:31.3
20:01:15.28 +30:37:51.6
19:58:38.18 +26:03:11.1
19:59:07.77 +31:19:42.1
19:58:22.47 +29:40:41.9
20:02:30.99 +32:07:12.0
19:58:00.42 +25:52:50.0
20:02:24.13 +25:50:51.5
19:59:53.18 +30:24:20.5
20:00:24.59 +30:54:02.9
19:58:02.07 +29:54:28.4
19:58:46.45 +29:48:34.4
19:58:14.81 +26:04:09.8
19:59:01.92 +29:12:32.7
19:58:20.07 +25:51:00.4
###################################################################################
19:55:42.18 +28:34:33.7 -- not an asteroid (will add it to exclusion list)
19:56:12.03 +29:14:46.0 -- not an asteroid (will add it to exclusion list)
19:59:01.94 +32:07:51.9 -- not an asteroid (will add it to exclusion list)
19:59:14.54 +25:54:46.8 -- not an asteroid (will add it to exclusion list)
19:59:27.23 +29:50:21.7 -- not an asteroid (will add it to exclusion list)
19:58:53.23 +29:45:03.1 -- not an asteroid (will add it to exclusion list)
19:55:47.57 +29:00:54.1 -- not an asteroid (will add it to exclusion list)
19:59:02.05 +30:00:13.6 -- not an asteroid (will add it to exclusion list)
19:56:08.65 +29:23:24.3 -- not an asteroid (will add it to exclusion list)
20:00:02.15 +30:51:15.2 -- not an asteroid (will add it to exclusion list)
19:58:57.04 +30:49:27.2 -- not an asteroid (will add it to exclusion list)
19:59:55.88 +30:43:52.0 -- not an asteroid (will add it to exclusion list)
20:00:01.36 +30:43:57.1 -- not an asteroid (will add it to exclusion list)
20:00:06.26 +30:27:25.4 -- not an asteroid (will add it to exclusion list)
20:00:07.21 +31:41:37.9 -- not an asteroid (will add it to exclusion list)
19:56:12.07 +28:39:49.7 -- not an asteroid (will add it to exclusion list)
19:58:49.33 +30:22:40.3 -- not an asteroid (will add it to exclusion list)
20:00:35.47 +31:04:10.7 -- not an asteroid (will add it to exclusion list)
19:58:22.20 +30:02:32.2 -- not an asteroid (will add it to exclusion list)
19:57:27.51 +29:32:41.4 -- not an asteroid (will add it to exclusion list)
19:57:39.51 +25:54:55.9 -- not an asteroid (will add it to exclusion list)
20:01:35.30 +30:39:54.5 -- not an asteroid (will add it to exclusion list)
19:59:43.57 +29:47:33.1 -- not an asteroid (will add it to exclusion list)
19:59:42.38 +30:46:18.0 -- not an asteroid (will add it to exclusion list)
19:59:02.01 +29:44:32.1 -- not an asteroid (will add it to exclusion list)
19:56:46.10 +29:12:02.6 -- not an asteroid (will add it to exclusion list)
20:00:12.42 +30:57:13.6 -- not an asteroid (will add it to exclusion list)
19:57:34.34 +25:52:41.3 -- not an asteroid (will add it to exclusion list)
19:56:00.81 +28:38:25.8 -- not an asteroid (will add it to exclusion list)
19:59:59.66 +31:58:05.8 -- not an asteroid (will add it to exclusion list)
19:58:13.35 +29:44:38.5 -- not an asteroid (will add it to exclusion list)
19:58:08.89 +30:27:26.6 -- not an asteroid (will add it to exclusion list)
19:59:06.15 +30:15:35.4 -- not an asteroid (will add it to exclusion list)
20:01:30.96 +30:19:16.6 -- not an asteroid (will add it to exclusion list)
19:59:31.92 +31:04:18.6 -- not an asteroid (will add it to exclusion list)
19:59:31.13 +30:57:10.4 -- not an asteroid (will add it to exclusion list)
20:01:38.22 +31:27:49.9 -- not an asteroid (will add it to exclusion list)
20:00:57.01 +25:59:35.3 -- not an asteroid (will add it to exclusion list)
19:56:49.81 +28:52:07.3 -- not an asteroid (will add it to exclusion list)
19:57:47.82 +29:07:01.6 -- not an asteroid (will add it to exclusion list)
20:02:12.23 +30:49:33.0 -- not an asteroid (will add it to exclusion list)
19:57:14.83 +28:55:17.9 -- not an asteroid (will add it to exclusion list)
20:02:44.28 +30:09:48.8 -- not an asteroid (will add it to exclusion list)
20:00:16.53 +29:17:15.9 -- not an asteroid (will add it to exclusion list)
20:02:18.84 +25:53:56.9 -- not an asteroid (will add it to exclusion list)
20:01:36.08 +31:04:07.4 -- not an asteroid (will add it to exclusion list)
19:57:05.99 +25:58:00.7 -- not an asteroid (will add it to exclusion list)
20:00:15.48 +30:25:29.9 -- not an asteroid (will add it to exclusion list)
19:53:33.24 +26:25:49.4 -- not an asteroid (will add it to exclusion list)
20:00:13.59 +31:31:48.2 -- not an asteroid (will add it to exclusion list)
20:00:26.88 +30:20:56.8 -- not an asteroid (will add it to exclusion list)
19:58:28.50 +25:46:25.3 -- not an asteroid (will add it to exclusion list)
19:59:05.35 +30:17:17.9 -- not an asteroid (will add it to exclusion list)
19:58:56.24 +30:04:00.0 -- not an asteroid (will add it to exclusion list)
19:57:52.09 +25:49:28.0 -- not an asteroid (will add it to exclusion list)
19:54:59.59 +25:52:13.3 -- not an asteroid (will add it to exclusion list)
19:57:33.00 +29:37:15.8 -- not an asteroid (will add it to exclusion list)
20:01:17.30 +25:52:51.8 -- not an asteroid (will add it to exclusion list)
20:01:50.92 +25:46:33.9 -- not an asteroid (will add it to exclusion list)
19:58:22.33 +29:57:37.3 -- not an asteroid (will add it to exclusion list)
20:02:05.32 +25:52:26.7 -- not an asteroid (will add it to exclusion list)
20:00:49.34 +30:03:56.3 -- not an asteroid (will add it to exclusion list)
19:53:31.30 +26:20:57.6 -- not an asteroid (will add it to exclusion list)
20:01:41.88 +26:12:07.5 -- not an asteroid (will add it to exclusion list)
19:58:19.70 +25:49:11.5 -- not an asteroid (will add it to exclusion list)
19:59:39.56 +25:55:00.5 -- not an asteroid (will add it to exclusion list)
20:01:56.56 +33:35:50.9 -- not an asteroid (will add it to exclusion list)
20:00:51.93 +25:49:06.9 -- not an asteroid (will add it to exclusion list)
20:00:49.22 +32:15:28.5 -- not an asteroid (will add it to exclusion list)
19:58:45.81 +25:54:26.8 -- not an asteroid (will add it to exclusion list)
19:57:41.93 +25:45:47.4 -- not an asteroid (will add it to exclusion list)
19:56:30.01 +25:46:24.1 -- not an asteroid (will add it to exclusion list)
20:00:48.41 +30:37:37.6 -- not an asteroid (will add it to exclusion list)
20:01:15.44 +30:23:20.1 -- not an asteroid (will add it to exclusion list)
19:59:02.39 +30:43:30.7 -- not an asteroid (will add it to exclusion list)
19:58:12.63 +30:30:42.9 -- not an asteroid (will add it to exclusion list)
20:02:07.55 +30:33:14.9 -- not an asteroid (will add it to exclusion list)
19:59:56.37 +32:24:56.1 -- not an asteroid (will add it to exclusion list)
19:54:49.28 +26:12:09.2 -- not an asteroid (will add it to exclusion list)
20:03:09.52 +30:01:38.4 -- not an asteroid (will add it to exclusion list)
19:58:21.53 +30:05:01.1 -- not an asteroid (will add it to exclusion list)
19:58:42.19 +25:50:16.2 -- not an asteroid (will add it to exclusion list)
20:00:09.95 +30:47:52.9 -- not an asteroid (will add it to exclusion list)
19:58:14.32 +29:22:03.3 -- not an asteroid (will add it to exclusion list)
19:58:50.92 +30:38:18.2 -- not an asteroid (will add it to exclusion list)
19:59:55.54 +31:12:18.6 -- not an asteroid (will add it to exclusion list)
19:58:06.90 +25:43:31.1 -- not an asteroid (will add it to exclusion list)
20:01:44.85 +30:36:59.9 -- not an asteroid (will add it to exclusion list)
19:59:22.85 +30:11:08.3 -- not an asteroid (will add it to exclusion list)
19:59:35.27 +30:06:32.3 -- not an asteroid (will add it to exclusion list)
20:00:15.72 +25:46:33.8 -- not an asteroid (will add it to exclusion list)
20:01:44.41 +33:21:00.5 -- not an asteroid (will add it to exclusion list)
19:57:12.81 +29:25:39.3 -- not an asteroid (will add it to exclusion list)
19:58:57.46 +25:49:51.1 -- not an asteroid (will add it to exclusion list)
19:58:19.27 +26:01:55.4 -- not an asteroid (will add it to exclusion list)
19:56:31.44 +29:05:41.9 -- not an asteroid (will add it to exclusion list)
20:00:30.25 +31:40:36.0 -- not an asteroid (will add it to exclusion list)
19:56:49.55 +28:54:45.5 -- not an asteroid (will add it to exclusion list)
20:01:44.93 +25:46:13.2 -- not an asteroid (will add it to exclusion list)
19:59:07.44 +29:36:00.5 -- not an asteroid (will add it to exclusion list)
20:02:10.36 +25:45:33.1 -- not an asteroid (will add it to exclusion list)
20:00:31.74 +31:51:06.3 -- not an asteroid (will add it to exclusion list)
19:58:26.78 +30:07:56.3 -- not an asteroid (will add it to exclusion list)
19:54:35.97 +25:52:08.6 -- not an asteroid (will add it to exclusion list)
20:00:35.55 +31:47:44.5 -- not an asteroid (will add it to exclusion list)
19:53:28.93 +25:57:40.5 -- not an asteroid (will add it to exclusion list)
19:59:21.96 +25:45:38.9 -- not an asteroid (will add it to exclusion list)
19:59:20.79 +31:19:32.0 -- not an asteroid (will add it to exclusion list)
19:57:48.62 +29:59:35.9 -- not an asteroid (will add it to exclusion list)
19:59:03.28 +30:47:12.5 -- not an asteroid (will add it to exclusion list)
20:00:13.73 +32:19:46.3 -- not an asteroid (will add it to exclusion list)
20:00:55.43 +31:15:31.2 -- not an asteroid (will add it to exclusion list)
19:53:25.38 +26:18:02.4 -- not an asteroid (will add it to exclusion list)
19:57:49.50 +25:59:41.9 -- not an asteroid (will add it to exclusion list)
20:00:22.78 +31:12:04.9 -- not an asteroid (will add it to exclusion list)
20:01:05.47 +30:29:15.8 -- not an asteroid (will add it to exclusion list)
19:57:29.34 +28:52:33.4 -- not an asteroid (will add it to exclusion list)
19:59:33.89 +31:00:18.8 -- not an asteroid (will add it to exclusion list)
19:59:48.91 +31:39:25.9 -- not an asteroid (will add it to exclusion list)
19:58:16.39 +30:21:22.8 -- not an asteroid (will add it to exclusion list)
19:58:41.31 +30:16:39.2 -- not an asteroid (will add it to exclusion list)
20:00:53.49 +30:40:33.3 -- not an asteroid (will add it to exclusion list)
19:55:27.67 +26:03:33.3 -- not an asteroid (will add it to exclusion list)
19:58:26.66 +29:33:48.2 -- not an asteroid (will add it to exclusion list)
19:57:43.61 +25:50:56.2 -- not an asteroid (will add it to exclusion list)
19:59:00.74 +25:45:38.7 -- not an asteroid (will add it to exclusion list)
19:55:41.39 +25:46:53.7 -- not an asteroid (will add it to exclusion list)
19:58:55.68 +29:48:04.0 -- not an asteroid (will add it to exclusion list)
20:01:21.70 +30:17:18.2 -- not an asteroid (will add it to exclusion list)
19:58:18.74 +30:34:52.9 -- not an asteroid (will add it to exclusion list)
19:54:56.77 +26:13:02.2 -- not an asteroid (will add it to exclusion list)
20:17:37.29 +26:53:19.4 -- not an asteroid (will add it to exclusion list)
19:59:25.11 +31:00:42.4 -- not an asteroid (will add it to exclusion list)
20:00:14.73 +31:15:57.2 -- not an asteroid (will add it to exclusion list)
19:58:52.56 +30:10:44.2 -- not an asteroid (will add it to exclusion list)
20:00:42.01 +31:22:50.4 -- not an asteroid (will add it to exclusion list)
20:00:26.60 +25:44:50.6 -- not an asteroid (will add it to exclusion list)
20:02:05.37 +33:25:18.5 -- not an asteroid (will add it to exclusion list)
19:57:31.57 +25:48:43.2 -- not an asteroid (will add it to exclusion list)
19:54:25.13 +26:04:08.8 -- not an asteroid (will add it to exclusion list)
19:59:18.72 +25:44:00.1 -- not an asteroid (will add it to exclusion list)
19:58:26.87 +29:45:35.7 -- not an asteroid (will add it to exclusion list)
19:59:42.53 +31:20:33.2 -- not an asteroid (will add it to exclusion list)
20:00:52.30 +30:56:27.2 -- not an asteroid (will add it to exclusion list)
19:58:08.13 +30:28:25.7 -- not an asteroid (will add it to exclusion list)
19:57:22.56 +25:52:20.0 -- not an asteroid (will add it to exclusion list)
20:00:02.00 +30:43:22.7 -- not an asteroid (will add it to exclusion list)
19:59:47.99 +29:47:38.9 -- not an asteroid (will add it to exclusion list)
19:59:44.95 +31:22:27.4 -- not an asteroid (will add it to exclusion list)
19:59:47.63 +31:26:08.0 -- not an asteroid (will add it to exclusion list)
20:01:13.82 +32:18:50.8 -- not an asteroid (will add it to exclusion list)
20:00:43.42 +30:58:10.9 -- not an asteroid (will add it to exclusion list)
19:54:11.00 +25:56:29.2 -- not an asteroid (will add it to exclusion list)
19:57:27.14 +25:53:16.0 -- not an asteroid (will add it to exclusion list)
20:00:45.08 +30:10:54.7 -- not an asteroid (will add it to exclusion list)
19:58:03.16 +29:31:38.0 -- not an asteroid (will add it to exclusion list)
19:58:03.83 +29:59:33.9 -- not an asteroid (will add it to exclusion list)
19:58:51.92 +25:50:54.6 -- not an asteroid (will add it to exclusion list)
20:02:33.38 +31:07:53.3 -- not an asteroid (will add it to exclusion list)
19:57:55.49 +29:35:05.8 -- not an asteroid (will add it to exclusion list)
19:59:17.68 +31:19:38.8 -- not an asteroid (will add it to exclusion list)
19:55:19.04 +25:46:36.7 -- not an asteroid (will add it to exclusion list)
19:56:28.94 +28:58:01.3 -- not an asteroid (will add it to exclusion list)
20:00:00.32 +31:15:01.3 -- not an asteroid (will add it to exclusion list)
19:55:14.97 +26:04:55.4 -- not an asteroid (will add it to exclusion list)
19:59:09.98 +29:43:59.5 -- not an asteroid (will add it to exclusion list)
19:59:20.09 +30:31:40.8 -- not an asteroid (will add it to exclusion list)
20:00:38.62 +25:58:43.6 -- not an asteroid (will add it to exclusion list)
20:01:04.18 +30:55:59.6 -- not an asteroid (will add it to exclusion list)
19:59:54.71 +31:15:44.6 -- not an asteroid (will add it to exclusion list)
20:02:46.86 +30:53:35.5 -- not an asteroid (will add it to exclusion list)
19:59:09.04 +25:48:35.8 -- not an asteroid (will add it to exclusion list)
20:00:36.60 +31:06:44.3 -- not an asteroid (will add it to exclusion list)
20:00:38.57 +25:46:05.9 -- not an asteroid (will add it to exclusion list)
19:58:29.02 +29:52:12.4 -- not an asteroid (will add it to exclusion list)
20:01:32.39 +30:38:28.9 -- not an asteroid (will add it to exclusion list)
20:00:02.54 +30:01:23.4 -- not an asteroid (will add it to exclusion list)
20:01:04.99 +30:23:00.4 -- not an asteroid (will add it to exclusion list)
19:55:46.85 +28:46:00.4 -- not an asteroid (will add it to exclusion list)
19:58:01.29 +25:49:54.8 -- not an asteroid (will add it to exclusion list)
19:59:29.59 +30:57:40.2 -- not an asteroid (will add it to exclusion list)
20:01:54.32 +30:45:43.8 -- not an asteroid (will add it to exclusion list)
20:00:48.54 +30:57:39.1 -- not an asteroid (will add it to exclusion list)
19:59:08.03 +30:19:59.8 -- not an asteroid (will add it to exclusion list)
19:59:15.68 +30:48:16.4 -- not an asteroid (will add it to exclusion list)
19:59:52.75 +31:07:20.5 -- not an asteroid (will add it to exclusion list)
19:58:54.86 +30:15:50.5 -- not an asteroid (will add it to exclusion list)
19:57:22.99 +29:38:30.4 -- not an asteroid (will add it to exclusion list)
19:59:07.95 +25:47:42.3 -- not an asteroid (will add it to exclusion list)
19:58:13.21 +25:48:33.1 -- not an asteroid (will add it to exclusion list)
19:55:17.20 +29:06:02.0 -- not an asteroid (will add it to exclusion list)
19:58:18.95 +29:58:29.4 -- not an asteroid (will add it to exclusion list)
20:00:36.18 +30:14:19.7 -- not an asteroid (will add it to exclusion list)
19:59:43.03 +31:55:48.6 -- not an asteroid (will add it to exclusion list)
19:59:59.29 +31:26:35.4 -- not an asteroid (will add it to exclusion list)
19:58:55.49 +30:52:15.4 -- not an asteroid (will add it to exclusion list)
19:55:01.22 +25:49:31.5 -- not an asteroid (will add it to exclusion list)
20:01:08.51 +30:40:44.1 -- not an asteroid (will add it to exclusion list)
19:59:11.96 +29:58:34.4 -- not an asteroid (will add it to exclusion list)
19:57:39.70 +29:55:32.9 -- not an asteroid (will add it to exclusion list)
19:59:29.60 +32:27:20.2 -- not an asteroid (will add it to exclusion list)
19:58:54.76 +30:13:37.9 -- not an asteroid (will add it to exclusion list)
19:53:39.52 +25:49:37.7 -- not an asteroid (will add it to exclusion list)
19:57:49.48 +25:45:29.6 -- not an asteroid (will add it to exclusion list)
20:00:34.10 +32:58:16.8 -- not an asteroid (will add it to exclusion list)
20:02:00.80 +30:45:35.1 -- not an asteroid (will add it to exclusion list)
19:59:42.83 +30:00:43.7 -- not an asteroid (will add it to exclusion list)
20:01:07.56 +29:35:24.2 -- not an asteroid (will add it to exclusion list)
19:58:45.69 +30:00:03.1 -- not an asteroid (will add it to exclusion list)
20:00:16.66 +30:31:25.4 -- not an asteroid (will add it to exclusion list)
19:56:45.22 +29:03:17.3 -- not an asteroid (will add it to exclusion list)
20:00:52.73 +29:45:24.0 -- not an asteroid (will add it to exclusion list)
19:55:22.66 +28:43:22.7 -- not an asteroid (will add it to exclusion list)
19:53:54.89 +26:09:26.5 -- not an asteroid (will add it to exclusion list)
20:01:47.39 +31:27:57.3 -- not an asteroid (will add it to exclusion list)
20:00:06.63 +31:57:06.3 -- not an asteroid (will add it to exclusion list)
19:57:24.87 +29:33:11.4 -- not an asteroid (will add it to exclusion list)
19:56:40.47 +28:47:29.5 -- not an asteroid (will add it to exclusion list)
19:54:59.82 +25:50:47.0 -- not an asteroid (will add it to exclusion list)
19:58:04.88 +29:55:30.9 -- not an asteroid (will add it to exclusion list)
20:02:12.80 +30:37:53.8 -- not an asteroid (will add it to exclusion list)
19:54:15.51 +25:56:25.6 -- not an asteroid (will add it to exclusion list)
20:00:37.48 +30:55:34.7 -- not an asteroid (will add it to exclusion list)
20:01:20.20 +31:12:16.0 -- not an asteroid (will add it to exclusion list)
19:56:58.18 +28:42:00.5 -- not an asteroid (will add it to exclusion list)
20:00:28.39 +30:42:05.3 -- not an asteroid (will add it to exclusion list)
20:00:34.21 +30:51:13.2 -- not an asteroid (will add it to exclusion list)
20:02:59.36 +30:19:08.0 -- not an asteroid (will add it to exclusion list)
19:56:31.43 +28:46:24.2 -- not an asteroid (will add it to exclusion list)
19:56:42.55 +25:50:11.6 -- not an asteroid (will add it to exclusion list)
19:58:40.90 +25:45:45.7 -- not an asteroid (will add it to exclusion list)
20:03:19.49 +25:51:04.5 -- not an asteroid (will add it to exclusion list)
19:57:19.44 +25:46:15.7 -- not an asteroid (will add it to exclusion list)
20:00:06.12 +30:58:39.6 -- not an asteroid (will add it to exclusion list)
19:54:46.74 +25:51:39.7 -- not an asteroid (will add it to exclusion list)
20:01:58.86 +30:15:36.8 -- not an asteroid (will add it to exclusion list)
20:00:27.70 +26:07:33.7 -- not an asteroid (will add it to exclusion list)
19:57:42.15 +25:46:08.2 -- not an asteroid (will add it to exclusion list)
19:59:14.40 +25:59:16.8 -- not an asteroid (will add it to exclusion list)
19:54:32.43 +25:47:23.1 -- not an asteroid (will add it to exclusion list)
19:52:58.12 +26:12:11.1 -- not an asteroid (will add it to exclusion list)
19:59:21.49 +29:43:58.4 -- not an asteroid (will add it to exclusion list)
19:54:44.94 +28:49:21.6 -- not an asteroid (will add it to exclusion list)
19:58:19.56 +30:13:37.2 -- not an asteroid (will add it to exclusion list)
20:01:01.33 +31:30:17.6 -- not an asteroid (will add it to exclusion list)
19:59:36.56 +25:55:06.1 -- not an asteroid (will add it to exclusion list)
19:58:07.93 +29:47:20.5 -- not an asteroid (will add it to exclusion list)
19:59:58.21 +30:58:22.3 -- not an asteroid (will add it to exclusion list)
19:59:04.74 +30:32:36.4 -- not an asteroid (will add it to exclusion list)
19:53:31.99 +26:01:32.9 -- not an asteroid (will add it to exclusion list)
20:02:06.14 +33:24:16.9 -- not an asteroid (will add it to exclusion list)
20:01:41.63 +31:00:41.3 -- not an asteroid (will add it to exclusion list)
20:00:35.11 +31:36:43.6 -- not an asteroid (will add it to exclusion list)
19:57:22.02 +29:19:28.2 -- not an asteroid (will add it to exclusion list)
19:58:15.88 +26:01:58.5 -- not an asteroid (will add it to exclusion list)
19:58:12.32 +25:57:27.2 -- not an asteroid (will add it to exclusion list)
19:58:25.41 +25:55:21.8 -- not an asteroid (will add it to exclusion list)
19:58:21.95 +29:55:36.4 -- not an asteroid (will add it to exclusion list)
19:59:55.27 +30:06:35.9 -- not an asteroid (will add it to exclusion list)
20:00:32.52 +30:48:48.7 -- not an asteroid (will add it to exclusion list)
19:55:23.76 +26:11:07.0 -- not an asteroid (will add it to exclusion list)
19:54:35.82 +26:11:51.5 -- not an asteroid (will add it to exclusion list)
20:02:36.32 +30:33:41.8 -- not an asteroid (will add it to exclusion list)
20:05:58.29 +29:56:16.7 -- not an asteroid (will add it to exclusion list)
19:59:50.70 +25:46:43.8 -- not an asteroid (will add it to exclusion list)
20:00:58.59 +30:35:14.3 -- not an asteroid (will add it to exclusion list)
19:59:02.58 +32:05:07.0 -- not an asteroid (will add it to exclusion list)
19:57:21.70 +26:00:42.0 -- not an asteroid (will add it to exclusion list)
20:01:06.84 +25:46:47.5 -- not an asteroid (will add it to exclusion list)
19:57:08.50 +29:24:21.4 -- not an asteroid (will add it to exclusion list)
19:57:44.32 +29:10:13.6 -- not an asteroid (will add it to exclusion list)
19:58:38.60 +31:24:27.8 -- not an asteroid (will add it to exclusion list)
19:58:52.11 +31:46:57.8 -- not an asteroid (will add it to exclusion list)
19:57:38.81 +31:34:58.3 -- not an asteroid (will add it to exclusion list)
19:57:37.43 +25:51:03.0 -- not an asteroid (will add it to exclusion list)
19:59:36.66 +30:48:43.4 -- not an asteroid (will add it to exclusion list)
19:55:53.90 +25:56:02.0 -- not an asteroid (will add it to exclusion list)
20:00:38.18 +30:48:34.7 -- not an asteroid (will add it to exclusion list)
19:57:18.37 +25:59:24.1 -- not an asteroid (will add it to exclusion list)
19:56:42.62 +29:35:47.2 -- not an asteroid (will add it to exclusion list)
19:59:09.14 +30:09:47.6 -- not an asteroid (will add it to exclusion list)
20:02:53.01 +32:31:41.7 -- not an asteroid (will add it to exclusion list)
19:54:32.12 +25:48:16.9 -- not an asteroid (will add it to exclusion list)
20:00:05.10 +31:12:28.3 -- not an asteroid (will add it to exclusion list)
20:00:46.53 +31:03:58.8 -- not an asteroid (will add it to exclusion list)
19:57:53.21 +29:28:32.3 -- not an asteroid (will add it to exclusion list)
19:54:25.21 +26:03:29.8 -- not an asteroid (will add it to exclusion list)
20:01:45.36 +26:04:16.3 -- not an asteroid (will add it to exclusion list)
19:57:34.69 +29:08:13.4 -- not an asteroid (will add it to exclusion list)
19:59:34.76 +29:55:24.1 -- not an asteroid (will add it to exclusion list)
19:59:49.89 +30:42:15.6 -- not an asteroid (will add it to exclusion list)
20:01:14.58 +26:09:44.5 -- not an asteroid (will add it to exclusion list)
19:57:04.06 +26:02:19.8 -- not an asteroid (will add it to exclusion list)
19:56:35.24 +28:47:50.4 -- not an asteroid (will add it to exclusion list)
19:58:23.69 +30:21:58.3 -- not an asteroid (will add it to exclusion list)
20:02:01.27 +25:47:24.0 -- not an asteroid (will add it to exclusion list)
20:00:12.46 +30:31:37.4 -- not an asteroid (will add it to exclusion list)
20:01:02.84 +30:43:29.0 -- not an asteroid (will add it to exclusion list)
19:56:40.48 +28:59:41.7 -- not an asteroid (will add it to exclusion list)
19:57:47.19 +29:44:05.7 -- not an asteroid (will add it to exclusion list)
19:56:48.33 +29:08:27.8 -- not an asteroid (will add it to exclusion list)
19:54:34.17 +25:54:28.8 -- not an asteroid (will add it to exclusion list)
20:00:03.59 +32:07:43.1 -- not an asteroid (will add it to exclusion list)
19:59:36.70 +30:59:57.5 -- not an asteroid (will add it to exclusion list)
20:00:19.41 +31:21:48.0 -- not an asteroid (will add it to exclusion list)
19:58:09.81 +30:29:46.0 -- not an asteroid (will add it to exclusion list)
19:58:46.52 +25:48:44.2 -- not an asteroid (will add it to exclusion list)
20:00:42.51 +30:25:21.0 -- not an asteroid (will add it to exclusion list)
19:59:41.47 +31:57:21.6 -- not an asteroid (will add it to exclusion list)
20:00:58.16 +31:15:25.4 -- not an asteroid (will add it to exclusion list)
19:59:32.10 +30:29:14.3 -- not an asteroid (will add it to exclusion list)
20:00:28.05 +31:32:04.9 -- not an asteroid (will add it to exclusion list)
20:00:49.81 +30:19:15.9 -- not an asteroid (will add it to exclusion list)
19:58:10.39 +25:52:58.3 -- not an asteroid (will add it to exclusion list)
19:58:27.05 +29:56:32.1 -- not an asteroid (will add it to exclusion list)
19:57:35.81 +29:13:08.8 -- not an asteroid (will add it to exclusion list)
19:57:53.05 +30:11:12.3 -- not an asteroid (will add it to exclusion list)
20:02:24.30 +30:19:20.6 -- not an asteroid (will add it to exclusion list)
19:54:46.96 +28:52:19.0 -- not an asteroid (will add it to exclusion list)
19:59:36.34 +25:47:45.6 -- not an asteroid (will add it to exclusion list)
19:54:07.40 +26:04:31.3 -- not an asteroid (will add it to exclusion list)
20:01:15.28 +30:37:51.6 -- not an asteroid (will add it to exclusion list)
19:58:38.18 +26:03:11.1 -- not an asteroid (will add it to exclusion list)
19:59:07.77 +31:19:42.1 -- not an asteroid (will add it to exclusion list)
19:58:22.47 +29:40:41.9 -- not an asteroid (will add it to exclusion list)
20:02:30.99 +32:07:12.0 -- not an asteroid (will add it to exclusion list)
19:58:00.42 +25:52:50.0 -- not an asteroid (will add it to exclusion list)
20:02:24.13 +25:50:51.5 -- not an asteroid (will add it to exclusion list)
19:59:53.18 +30:24:20.5 -- not an asteroid (will add it to exclusion list)
20:00:24.59 +30:54:02.9 -- not an asteroid (will add it to exclusion list)
19:58:02.07 +29:54:28.4 -- not an asteroid (will add it to exclusion list)
19:58:46.45 +29:48:34.4 -- not an asteroid (will add it to exclusion list)
19:58:14.81 +26:04:09.8 -- not an asteroid (will add it to exclusion list)
19:59:01.92 +29:12:32.7 -- not an asteroid (will add it to exclusion list)
19:58:20.07 +25:51:00.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:52:58.12 +26:12:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:25.38 +26:18:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:28.93 +25:57:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:31.30 +26:20:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:31.99 +26:01:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:33.24 +26:25:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:39.52 +25:49:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:54.89 +26:09:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:07.40 +26:04:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:11.00 +25:56:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:15.51 +25:56:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:25.13 +26:04:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:25.21 +26:03:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:32.12 +25:48:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:32.43 +25:47:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:34.17 +25:54:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:35.82 +26:11:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:35.97 +25:52:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:44.94 +28:49:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:46.74 +25:51:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:46.96 +28:52:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:49.28 +26:12:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:56.77 +26:13:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:59.59 +25:52:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:59.82 +25:50:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:01.22 +25:49:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:14.97 +26:04:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:17.20 +29:06:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:19.04 +25:46:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:22.66 +28:43:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:23.76 +26:11:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:27.67 +26:03:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:41.39 +25:46:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:42.18 +28:34:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:46.85 +28:46:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:47.57 +29:00:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:53.90 +25:56:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:00.81 +28:38:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:08.65 +29:23:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:12.03 +29:14:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:12.07 +28:39:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:28.94 +28:58:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:30.01 +25:46:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:31.43 +28:46:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:31.44 +29:05:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:35.24 +28:47:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:40.47 +28:47:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:40.48 +28:59:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:42.55 +25:50:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:42.62 +29:35:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:45.22 +29:03:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:46.10 +29:12:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:48.33 +29:08:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:49.55 +28:54:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:49.81 +28:52:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:58.18 +28:42:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:04.06 +26:02:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:05.99 +25:58:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:08.50 +29:24:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:12.81 +29:25:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:14.83 +28:55:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:18.37 +25:59:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:19.44 +25:46:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:21.70 +26:00:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:22.02 +29:19:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:22.56 +25:52:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:22.99 +29:38:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:24.87 +29:33:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:27.14 +25:53:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:27.51 +29:32:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:29.34 +28:52:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:31.57 +25:48:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:33.00 +29:37:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:34.34 +25:52:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:34.69 +29:08:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:35.81 +29:13:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:37.43 +25:51:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:38.81 +31:34:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:39.51 +25:54:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:39.70 +29:55:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:41.93 +25:45:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:42.15 +25:46:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:43.61 +25:50:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:44.32 +29:10:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:47.19 +29:44:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:47.82 +29:07:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:48.62 +29:59:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:49.48 +25:45:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:49.50 +25:59:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:52.09 +25:49:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:53.05 +30:11:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:53.21 +29:28:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:55.49 +29:35:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:00.42 +25:52:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:01.29 +25:49:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:02.07 +29:54:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:03.16 +29:31:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:03.83 +29:59:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:04.88 +29:55:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:06.90 +25:43:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:07.93 +29:47:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:08.13 +30:28:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:08.89 +30:27:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:09.81 +30:29:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:10.39 +25:52:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:12.32 +25:57:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:12.63 +30:30:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:13.21 +25:48:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:13.35 +29:44:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:14.32 +29:22:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:14.81 +26:04:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:15.88 +26:01:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:16.39 +30:21:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:18.74 +30:34:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:18.95 +29:58:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:19.27 +26:01:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:19.56 +30:13:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:19.70 +25:49:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:20.07 +25:51:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:21.53 +30:05:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:21.95 +29:55:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:22.20 +30:02:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:22.33 +29:57:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:22.47 +29:40:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:23.69 +30:21:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:25.41 +25:55:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:26.66 +29:33:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:26.78 +30:07:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:26.87 +29:45:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:27.05 +29:56:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:28.50 +25:46:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:29.02 +29:52:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:38.18 +26:03:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:38.60 +31:24:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:40.90 +25:45:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:41.31 +30:16:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:42.19 +25:50:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:45.69 +30:00:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:45.81 +25:54:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:46.45 +29:48:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:46.52 +25:48:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:49.33 +30:22:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:50.92 +30:38:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:51.92 +25:50:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:52.11 +31:46:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:52.56 +30:10:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:53.23 +29:45:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:54.76 +30:13:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:54.86 +30:15:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:55.49 +30:52:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:55.68 +29:48:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:56.24 +30:04:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:57.04 +30:49:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:57.46 +25:49:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:00.74 +25:45:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:01.92 +29:12:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:01.94 +32:07:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:02.01 +29:44:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:02.05 +30:00:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:02.39 +30:43:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:02.58 +32:05:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:03.28 +30:47:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:04.74 +30:32:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:05.35 +30:17:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:06.15 +30:15:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:07.44 +29:36:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:07.77 +31:19:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:07.95 +25:47:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:08.03 +30:19:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:09.04 +25:48:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:09.14 +30:09:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:09.98 +29:43:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:11.96 +29:58:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:14.40 +25:59:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:14.54 +25:54:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:15.68 +30:48:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:17.68 +31:19:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:18.72 +25:44:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:20.09 +30:31:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:20.79 +31:19:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:21.49 +29:43:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:21.96 +25:45:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:22.85 +30:11:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:25.11 +31:00:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:27.23 +29:50:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:29.59 +30:57:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:29.60 +32:27:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:31.13 +30:57:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:31.92 +31:04:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:32.10 +30:29:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:33.89 +31:00:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:34.76 +29:55:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:35.27 +30:06:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:36.34 +25:47:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:36.56 +25:55:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:36.66 +30:48:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:36.70 +30:59:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:39.56 +25:55:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:41.47 +31:57:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:42.38 +30:46:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:42.53 +31:20:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:42.83 +30:00:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:43.03 +31:55:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:43.57 +29:47:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:44.95 +31:22:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:47.63 +31:26:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:47.99 +29:47:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:48.91 +31:39:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:49.89 +30:42:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:50.70 +25:46:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:52.75 +31:07:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:53.18 +30:24:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:54.71 +31:15:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:55.27 +30:06:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:55.54 +31:12:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:55.88 +30:43:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:56.37 +32:24:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:58.21 +30:58:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:59.29 +31:26:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:59.66 +31:58:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:00.32 +31:15:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:01.36 +30:43:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:02.00 +30:43:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:02.15 +30:51:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:02.54 +30:01:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:03.59 +32:07:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:05.10 +31:12:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:06.12 +30:58:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:06.26 +30:27:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:06.63 +31:57:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:07.21 +31:41:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:09.95 +30:47:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:12.42 +30:57:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:12.46 +30:31:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:13.59 +31:31:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:13.73 +32:19:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:14.73 +31:15:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:15.48 +30:25:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:15.72 +25:46:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:16.53 +29:17:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:16.66 +30:31:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:19.41 +31:21:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:22.78 +31:12:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:24.59 +30:54:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:26.60 +25:44:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:26.88 +30:20:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:27.70 +26:07:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:28.05 +31:32:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:28.39 +30:42:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:30.25 +31:40:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:31.74 +31:51:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:32.52 +30:48:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:34.10 +32:58:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:34.21 +30:51:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:35.11 +31:36:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:35.47 +31:04:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:35.55 +31:47:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:36.18 +30:14:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:36.60 +31:06:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:37.48 +30:55:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:38.18 +30:48:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:38.57 +25:46:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:38.62 +25:58:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:42.01 +31:22:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:42.51 +30:25:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:43.42 +30:58:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:45.08 +30:10:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:46.53 +31:03:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:48.41 +30:37:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:48.54 +30:57:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:49.22 +32:15:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:49.34 +30:03:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:49.81 +30:19:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:51.93 +25:49:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:52.30 +30:56:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:52.73 +29:45:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:53.49 +30:40:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:55.43 +31:15:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:57.01 +25:59:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:58.16 +31:15:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:58.59 +30:35:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:01.33 +31:30:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:02.84 +30:43:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:04.18 +30:55:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:04.99 +30:23:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:05.47 +30:29:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:06.84 +25:46:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:07.56 +29:35:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:08.51 +30:40:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:13.82 +32:18:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:14.58 +26:09:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:15.28 +30:37:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:15.44 +30:23:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:17.30 +25:52:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:20.20 +31:12:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:21.70 +30:17:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:30.96 +30:19:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:32.39 +30:38:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:35.30 +30:39:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:36.08 +31:04:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:38.22 +31:27:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:41.63 +31:00:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:41.88 +26:12:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:44.41 +33:21:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:44.85 +30:36:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:44.93 +25:46:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:45.36 +26:04:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:47.39 +31:27:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:50.92 +25:46:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:54.32 +30:45:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:56.56 +33:35:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:58.86 +30:15:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:00.80 +30:45:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:01.27 +25:47:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:05.32 +25:52:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:05.37 +33:25:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:06.14 +33:24:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:07.55 +30:33:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:10.36 +25:45:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:12.23 +30:49:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:12.80 +30:37:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:18.84 +25:53:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:24.13 +25:50:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:24.30 +30:19:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:30.99 +32:07:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:33.38 +31:07:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:36.32 +30:33:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:44.28 +30:09:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:46.86 +30:53:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:53.01 +32:31:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:59.36 +30:19:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:09.52 +30:01:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:19.49 +25:51:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:58.29 +29:56:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:37.29 +26:53:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
19:52:58.12 +26:12:11.1 -- not a known variable star
19:53:25.38 +26:18:02.4 -- not a known variable star
19:53:28.93 +25:57:40.5 -- not a known variable star
19:53:31.30 +26:20:57.6 -- not a known variable star
19:53:31.99 +26:01:32.9 -- not a known variable star
19:53:33.24 +26:25:49.4 -- not a known variable star
19:53:39.52 +25:49:37.7 -- not a known variable star
19:53:54.89 +26:09:26.5 -- not a known variable star
19:54:07.40 +26:04:31.3 -- a known variable star
19:54:11.00 +25:56:29.2 -- a known variable star
19:54:15.51 +25:56:25.6 -- not a known variable star
19:54:25.13 +26:04:08.8 -- not a known variable star
19:54:25.21 +26:03:29.8 -- not a known variable star
19:54:32.12 +25:48:16.9 -- not a known variable star
19:54:32.43 +25:47:23.1 -- not a known variable star
19:54:34.17 +25:54:28.8 -- a known variable star
19:54:35.82 +26:11:51.5 -- not a known variable star
19:54:35.97 +25:52:08.6 -- not a known variable star
19:54:44.94 +28:49:21.6 -- a known variable star
19:54:46.74 +25:51:39.7 -- a known variable star
19:54:46.96 +28:52:19.0 -- a known variable star
19:54:49.28 +26:12:09.2 -- not a known variable star
19:54:56.77 +26:13:02.2 -- a known variable star
19:54:59.59 +25:52:13.3 -- a known variable star
19:54:59.82 +25:50:47.0 -- not a known variable star
19:55:01.22 +25:49:31.5 -- not a known variable star
19:55:14.97 +26:04:55.4 -- not a known variable star
19:55:17.20 +29:06:02.0 -- not a known variable star
19:55:19.04 +25:46:36.7 -- not a known variable star
19:55:22.66 +28:43:22.7 -- a known variable star
19:55:23.76 +26:11:07.0 -- not a known variable star
19:55:27.67 +26:03:33.3 -- not a known variable star
19:55:41.39 +25:46:53.7 -- not a known variable star
19:55:42.18 +28:34:33.7 -- not a known variable star
19:55:46.85 +28:46:00.4 -- a known variable star
19:55:47.57 +29:00:54.1 -- not a known variable star
19:55:53.90 +25:56:02.0 -- not a known variable star
19:56:00.81 +28:38:25.8 -- a known variable star
19:56:08.65 +29:23:24.3 -- not a known variable star
19:56:12.03 +29:14:46.0 -- not a known variable star
19:56:12.07 +28:39:49.7 -- a known variable star
19:56:28.94 +28:58:01.3 -- not a known variable star
19:56:30.01 +25:46:24.1 -- not a known variable star
19:56:31.43 +28:46:24.2 -- a known variable star
19:56:31.44 +29:05:41.9 -- not a known variable star
19:56:35.24 +28:47:50.4 -- not a known variable star
19:56:40.47 +28:47:29.5 -- not a known variable star
19:56:40.48 +28:59:41.7 -- not a known variable star
19:56:42.55 +25:50:11.6 -- not a known variable star
19:56:42.62 +29:35:47.2 -- not a known variable star
19:56:45.22 +29:03:17.3 -- not a known variable star
19:56:46.10 +29:12:02.6 -- not a known variable star
19:56:48.33 +29:08:27.8 -- not a known variable star
19:56:49.55 +28:54:45.5 -- not a known variable star
19:56:49.81 +28:52:07.3 -- not a known variable star
19:56:58.18 +28:42:00.5 -- not a known variable star
19:57:04.06 +26:02:19.8 -- not a known variable star
19:57:05.99 +25:58:00.7 -- not a known variable star
19:57:08.50 +29:24:21.4 -- a known variable star
19:57:12.81 +29:25:39.3 -- not a known variable star
19:57:14.83 +28:55:17.9 -- not a known variable star
19:57:18.37 +25:59:24.1 -- not a known variable star
19:57:19.44 +25:46:15.7 -- not a known variable star
19:57:21.70 +26:00:42.0 -- not a known variable star
19:57:22.02 +29:19:28.2 -- not a known variable star
19:57:22.56 +25:52:20.0 -- a known variable star
19:57:22.99 +29:38:30.4 -- not a known variable star
19:57:24.87 +29:33:11.4 -- not a known variable star
19:57:27.14 +25:53:16.0 -- not a known variable star
19:57:27.51 +29:32:41.4 -- not a known variable star
19:57:29.34 +28:52:33.4 -- not a known variable star
19:57:31.57 +25:48:43.2 -- not a known variable star
19:57:33.00 +29:37:15.8 -- not a known variable star
19:57:34.34 +25:52:41.3 -- a known variable star
19:57:34.69 +29:08:13.4 -- not a known variable star
19:57:35.81 +29:13:08.8 -- a known variable star
19:57:37.43 +25:51:03.0 -- not a known variable star
19:57:38.81 +31:34:58.3 -- not a known variable star
19:57:39.51 +25:54:55.9 -- a known variable star
19:57:39.70 +29:55:32.9 -- not a known variable star
19:57:41.93 +25:45:47.4 -- not a known variable star
19:57:42.15 +25:46:08.2 -- a known variable star
19:57:43.61 +25:50:56.2 -- not a known variable star
19:57:44.32 +29:10:13.6 -- not a known variable star
19:57:47.19 +29:44:05.7 -- a known variable star
19:57:47.82 +29:07:01.6 -- a known variable star
19:57:48.62 +29:59:35.9 -- not a known variable star
19:57:49.48 +25:45:29.6 -- a known variable star
19:57:49.50 +25:59:41.9 -- not a known variable star
19:57:52.09 +25:49:28.0 -- not a known variable star
19:57:53.05 +30:11:12.3 -- not a known variable star
19:57:53.21 +29:28:32.3 -- not a known variable star
19:57:55.49 +29:35:05.8 -- not a known variable star
19:58:00.42 +25:52:50.0 -- not a known variable star
19:58:01.29 +25:49:54.8 -- not a known variable star
19:58:02.07 +29:54:28.4 -- not a known variable star
19:58:03.16 +29:31:38.0 -- a known variable star
19:58:03.83 +29:59:33.9 -- a known variable star
19:58:04.88 +29:55:30.9 -- not a known variable star
19:58:06.90 +25:43:31.1 -- not a known variable star
19:58:07.93 +29:47:20.5 -- a known variable star
19:58:08.13 +30:28:25.7 -- not a known variable star
19:58:08.89 +30:27:26.6 -- not a known variable star
19:58:09.81 +30:29:46.0 -- not a known variable star
19:58:10.39 +25:52:58.3 -- not a known variable star
19:58:12.32 +25:57:27.2 -- a known variable star
19:58:12.63 +30:30:42.9 -- not a known variable star
19:58:13.21 +25:48:33.1 -- not a known variable star
19:58:13.35 +29:44:38.5 -- not a known variable star
19:58:14.32 +29:22:03.3 -- not a known variable star
19:58:14.81 +26:04:09.8 -- not a known variable star
19:58:15.88 +26:01:58.5 -- a known variable star
19:58:16.39 +30:21:22.8 -- a known variable star
19:58:18.74 +30:34:52.9 -- a known variable star
19:58:18.95 +29:58:29.4 -- not a known variable star
19:58:19.27 +26:01:55.4 -- not a known variable star
19:58:19.56 +30:13:37.2 -- not a known variable star
19:58:19.70 +25:49:11.5 -- a known variable star
19:58:20.07 +25:51:00.4 -- not a known variable star
19:58:21.53 +30:05:01.1 -- not a known variable star
19:58:21.95 +29:55:36.4 -- a known variable star
19:58:22.20 +30:02:32.2 -- a known variable star
19:58:22.33 +29:57:37.3 -- a known variable star
19:58:22.47 +29:40:41.9 -- not a known variable star
19:58:23.69 +30:21:58.3 -- not a known variable star
19:58:25.41 +25:55:21.8 -- not a known variable star
19:58:26.66 +29:33:48.2 -- not a known variable star
19:58:26.78 +30:07:56.3 -- not a known variable star
19:58:26.87 +29:45:35.7 -- not a known variable star
19:58:27.05 +29:56:32.1 -- not a known variable star
19:58:28.50 +25:46:25.3 -- not a known variable star
19:58:29.02 +29:52:12.4 -- not a known variable star
19:58:38.18 +26:03:11.1 -- not a known variable star
19:58:38.60 +31:24:27.8 -- not a known variable star
19:58:40.90 +25:45:45.7 -- a known variable star
19:58:41.31 +30:16:39.2 -- not a known variable star
19:58:42.19 +25:50:16.2 -- not a known variable star
19:58:45.69 +30:00:03.1 -- a known variable star
19:58:45.81 +25:54:26.8 -- not a known variable star
19:58:46.45 +29:48:34.4 -- not a known variable star
19:58:46.52 +25:48:44.2 -- not a known variable star
19:58:49.33 +30:22:40.3 -- not a known variable star
19:58:50.92 +30:38:18.2 -- not a known variable star
19:58:51.92 +25:50:54.6 -- not a known variable star
19:58:52.11 +31:46:57.8 -- a known variable star
19:58:52.56 +30:10:44.2 -- not a known variable star
19:58:53.23 +29:45:03.1 -- a known variable star
19:58:54.76 +30:13:37.9 -- a known variable star
19:58:54.86 +30:15:50.5 -- a known variable star
19:58:55.49 +30:52:15.4 -- a known variable star
19:58:55.68 +29:48:04.0 -- a known variable star
19:58:56.24 +30:04:00.0 -- not a known variable star
19:58:57.04 +30:49:27.2 -- not a known variable star
19:58:57.46 +25:49:51.1 -- not a known variable star
19:59:00.74 +25:45:38.7 -- not a known variable star
19:59:01.92 +29:12:32.7 -- a known variable star
19:59:01.94 +32:07:51.9 -- not a known variable star
19:59:02.01 +29:44:32.1 -- not a known variable star
19:59:02.05 +30:00:13.6 -- not a known variable star
19:59:02.39 +30:43:30.7 -- not a known variable star
19:59:02.58 +32:05:07.0 -- not a known variable star
19:59:03.28 +30:47:12.5 -- not a known variable star
19:59:04.74 +30:32:36.4 -- a known variable star
19:59:05.35 +30:17:17.9 -- not a known variable star
19:59:06.15 +30:15:35.4 -- not a known variable star
19:59:07.44 +29:36:00.5 -- a known variable star
19:59:07.77 +31:19:42.1 -- a known variable star
19:59:07.95 +25:47:42.3 -- not a known variable star
19:59:08.03 +30:19:59.8 -- not a known variable star
19:59:09.04 +25:48:35.8 -- not a known variable star
19:59:09.14 +30:09:47.6 -- not a known variable star
19:59:09.98 +29:43:59.5 -- a known variable star
19:59:11.96 +29:58:34.4 -- not a known variable star
19:59:14.40 +25:59:16.8 -- not a known variable star
19:59:14.54 +25:54:46.8 -- a known variable star
19:59:15.68 +30:48:16.4 -- not a known variable star
19:59:17.68 +31:19:38.8 -- not a known variable star
19:59:18.72 +25:44:00.1 -- not a known variable star
19:59:20.09 +30:31:40.8 -- not a known variable star
19:59:20.79 +31:19:32.0 -- not a known variable star
19:59:21.49 +29:43:58.4 -- a known variable star
19:59:21.96 +25:45:38.9 -- not a known variable star
19:59:22.85 +30:11:08.3 -- a known variable star
19:59:25.11 +31:00:42.4 -- not a known variable star
19:59:27.23 +29:50:21.7 -- not a known variable star
19:59:29.59 +30:57:40.2 -- not a known variable star
19:59:29.60 +32:27:20.2 -- not a known variable star
19:59:31.13 +30:57:10.4 -- a known variable star
19:59:31.92 +31:04:18.6 -- a known variable star
19:59:32.10 +30:29:14.3 -- a known variable star
19:59:33.89 +31:00:18.8 -- a known variable star
19:59:34.76 +29:55:24.1 -- not a known variable star
19:59:35.27 +30:06:32.3 -- a known variable star
19:59:36.34 +25:47:45.6 -- not a known variable star
19:59:36.56 +25:55:06.1 -- not a known variable star
19:59:36.66 +30:48:43.4 -- a known variable star
19:59:36.70 +30:59:57.5 -- not a known variable star
19:59:39.56 +25:55:00.5 -- a known variable star
19:59:41.47 +31:57:21.6 -- not a known variable star
19:59:42.38 +30:46:18.0 -- not a known variable star
19:59:42.53 +31:20:33.2 -- not a known variable star
19:59:42.83 +30:00:43.7 -- a known variable star
19:59:43.03 +31:55:48.6 -- not a known variable star
19:59:43.57 +29:47:33.1 -- not a known variable star
19:59:44.95 +31:22:27.4 -- not a known variable star
19:59:47.63 +31:26:08.0 -- not a known variable star
19:59:47.99 +29:47:38.9 -- not a known variable star
19:59:48.91 +31:39:25.9 -- not a known variable star
19:59:49.89 +30:42:15.6 -- not a known variable star
19:59:50.70 +25:46:43.8 -- not a known variable star
19:59:52.75 +31:07:20.5 -- not a known variable star
19:59:53.18 +30:24:20.5 -- a known variable star
19:59:54.71 +31:15:44.6 -- not a known variable star
19:59:55.27 +30:06:35.9 -- not a known variable star
19:59:55.54 +31:12:18.6 -- a known variable star
19:59:55.88 +30:43:52.0 -- not a known variable star
19:59:56.37 +32:24:56.1 -- not a known variable star
19:59:58.21 +30:58:22.3 -- not a known variable star
19:59:59.29 +31:26:35.4 -- not a known variable star
19:59:59.66 +31:58:05.8 -- not a known variable star
20:00:00.32 +31:15:01.3 -- not a known variable star
20:00:01.36 +30:43:57.1 -- not a known variable star
20:00:02.00 +30:43:22.7 -- not a known variable star
20:00:02.15 +30:51:15.2 -- a known variable star
20:00:02.54 +30:01:23.4 -- not a known variable star
20:00:03.59 +32:07:43.1 -- not a known variable star
20:00:05.10 +31:12:28.3 -- not a known variable star
20:00:06.12 +30:58:39.6 -- not a known variable star
20:00:06.26 +30:27:25.4 -- a known variable star
20:00:06.63 +31:57:06.3 -- not a known variable star
20:00:07.21 +31:41:37.9 -- a known variable star
20:00:09.95 +30:47:52.9 -- a known variable star
20:00:12.42 +30:57:13.6 -- not a known variable star
20:00:12.46 +30:31:37.4 -- a known variable star
20:00:13.59 +31:31:48.2 -- a known variable star
20:00:13.73 +32:19:46.3 -- not a known variable star
20:00:14.73 +31:15:57.2 -- not a known variable star
20:00:15.48 +30:25:29.9 -- not a known variable star
20:00:15.72 +25:46:33.8 -- a known variable star
20:00:16.53 +29:17:15.9 -- a known variable star
20:00:16.66 +30:31:25.4 -- not a known variable star
20:00:19.41 +31:21:48.0 -- not a known variable star
20:00:22.78 +31:12:04.9 -- not a known variable star
20:00:24.59 +30:54:02.9 -- not a known variable star
20:00:26.60 +25:44:50.6 -- not a known variable star
20:00:26.88 +30:20:56.8 -- a known variable star
20:00:27.70 +26:07:33.7 -- not a known variable star
20:00:28.05 +31:32:04.9 -- not a known variable star
20:00:28.39 +30:42:05.3 -- not a known variable star
20:00:30.25 +31:40:36.0 -- not a known variable star
20:00:31.74 +31:51:06.3 -- not a known variable star
20:00:32.52 +30:48:48.7 -- a known variable star
20:00:34.10 +32:58:16.8 -- a known variable star
20:00:34.21 +30:51:13.2 -- not a known variable star
20:00:35.11 +31:36:43.6 -- not a known variable star
20:00:35.47 +31:04:10.7 -- not a known variable star
20:00:35.55 +31:47:44.5 -- a known variable star
20:00:36.18 +30:14:19.7 -- not a known variable star
20:00:36.60 +31:06:44.3 -- not a known variable star
20:00:37.48 +30:55:34.7 -- not a known variable star
20:00:38.18 +30:48:34.7 -- not a known variable star
20:00:38.57 +25:46:05.9 -- not a known variable star
20:00:38.62 +25:58:43.6 -- not a known variable star
20:00:42.01 +31:22:50.4 -- a known variable star
20:00:42.51 +30:25:21.0 -- a known variable star
20:00:43.42 +30:58:10.9 -- not a known variable star
20:00:45.08 +30:10:54.7 -- not a known variable star
20:00:46.53 +31:03:58.8 -- not a known variable star
20:00:48.41 +30:37:37.6 -- not a known variable star
20:00:48.54 +30:57:39.1 -- not a known variable star
20:00:49.22 +32:15:28.5 -- not a known variable star
20:00:49.34 +30:03:56.3 -- a known variable star
20:00:49.81 +30:19:15.9 -- not a known variable star
20:00:51.93 +25:49:06.9 -- not a known variable star
20:00:52.30 +30:56:27.2 -- not a known variable star
20:00:52.73 +29:45:24.0 -- not a known variable star
20:00:53.49 +30:40:33.3 -- a known variable star
20:00:55.43 +31:15:31.2 -- not a known variable star
20:00:57.01 +25:59:35.3 -- not a known variable star
20:00:58.16 +31:15:25.4 -- not a known variable star
20:00:58.59 +30:35:14.3 -- not a known variable star
20:01:01.33 +31:30:17.6 -- not a known variable star
20:01:02.84 +30:43:29.0 -- not a known variable star
20:01:04.18 +30:55:59.6 -- not a known variable star
20:01:04.99 +30:23:00.4 -- a known variable star
20:01:05.47 +30:29:15.8 -- not a known variable star
20:01:06.84 +25:46:47.5 -- not a known variable star
20:01:07.56 +29:35:24.2 -- a known variable star
20:01:08.51 +30:40:44.1 -- not a known variable star
20:01:13.82 +32:18:50.8 -- a known variable star
20:01:14.58 +26:09:44.5 -- not a known variable star
20:01:15.28 +30:37:51.6 -- not a known variable star
20:01:15.44 +30:23:20.1 -- not a known variable star
20:01:17.30 +25:52:51.8 -- not a known variable star
20:01:20.20 +31:12:16.0 -- not a known variable star
20:01:21.70 +30:17:18.2 -- not a known variable star
20:01:30.96 +30:19:16.6 -- not a known variable star
20:01:32.39 +30:38:28.9 -- not a known variable star
20:01:35.30 +30:39:54.5 -- not a known variable star
20:01:36.08 +31:04:07.4 -- not a known variable star
20:01:38.22 +31:27:49.9 -- not a known variable star
20:01:41.63 +31:00:41.3 -- not a known variable star
20:01:41.88 +26:12:07.5 -- a known variable star
20:01:44.41 +33:21:00.5 -- not a known variable star
20:01:44.85 +30:36:59.9 -- not a known variable star
20:01:44.93 +25:46:13.2 -- a known variable star
20:01:45.36 +26:04:16.3 -- not a known variable star
20:01:47.39 +31:27:57.3 -- not a known variable star
20:01:50.92 +25:46:33.9 -- not a known variable star
20:01:54.32 +30:45:43.8 -- not a known variable star
20:01:56.56 +33:35:50.9 -- a known variable star
20:01:58.86 +30:15:36.8 -- a known variable star
20:02:00.80 +30:45:35.1 -- not a known variable star
20:02:01.27 +25:47:24.0 -- a known variable star
20:02:05.32 +25:52:26.7 -- not a known variable star
20:02:05.37 +33:25:18.5 -- not a known variable star
20:02:06.14 +33:24:16.9 -- a known variable star
20:02:07.55 +30:33:14.9 -- a known variable star
20:02:10.36 +25:45:33.1 -- not a known variable star
20:02:12.23 +30:49:33.0 -- a known variable star
20:02:12.80 +30:37:53.8 -- not a known variable star
20:02:18.84 +25:53:56.9 -- not a known variable star
20:02:24.13 +25:50:51.5 -- not a known variable star
20:02:24.30 +30:19:20.6 -- not a known variable star
20:02:30.99 +32:07:12.0 -- a known variable star
20:02:33.38 +31:07:53.3 -- not a known variable star
20:02:36.32 +30:33:41.8 -- not a known variable star
20:02:44.28 +30:09:48.8 -- not a known variable star
20:02:46.86 +30:53:35.5 -- not a known variable star
20:02:53.01 +32:31:41.7 -- a known variable star
20:02:59.36 +30:19:08.0 -- a known variable star
20:03:09.52 +30:01:38.4 -- not a known variable star
20:03:19.49 +25:51:04.5 -- a known variable star
20:05:58.29 +29:56:16.7 -- not a known variable star
20:17:37.29 +26:53:19.4 -- a known variable star
Found 244 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
335 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 335 (excluding asteroids and hot pixels, 244 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
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461199.66992943 -observatory V36
06:43:36.21 +25:00:19.5 Mercury (0.1mag)
07:42:44.56 +23:23:01.7 Venus (-4.0mag)
02:49:32.70 +15:42:32.7 Mars (1.3mag)
07:48:25.15 +21:31:29.9 Jupiter (-1.9mag)
00:49:22.07 +02:48:38.8 Saturn (0.9mag)
04:00:12.09 +20:25:26.9 Uranus (5.8mag)
00:16:08.46 +00:16:47.9 Neptune (7.8mag)
20:33:21.47 -23:04:32.3 Pluto (14.5mag)
23:02:07.08 -05:46:55.2 Moon (-10.4mag)
-rw-r--r-- 1 apache apache 362 Jun 8 00:14 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461199.66992943:
07:48:25.69 +21:31:30.5 Io (6.0mag)
07:48:25.08 +21:31:32.3 Europa (6.2mag)
07:48:09.25 +21:32:17.2 Ganymede (5.6mag)
07:48:43.93 +21:30:29.4 Callisto (6.7mag)
07:48:42.58 +21:07:47.5 Himalia (15.6mag)
07:48:29.72 +21:31:15.9 Thebe (16.5mag)
07:48:42.06 +21:23:14.6 Elara (17.5mag)
07:50:35.77 +21:43:12.5 Pasiphae (17.7mag)
07:55:00.29 +21:33:12.3 Carme (18.9mag)
00:49:12.60 +02:48:37.8 Titan (8.7mag)
00:49:19.07 +02:48:52.1 Rhea (9.9mag)
00:49:54.36 +02:50:48.1 Iapetus (11.3mag)
00:49:17.98 +02:48:15.9 Hyperion (14.7mag)
00:50:04.36 +02:50:35.6 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 568 Jun 8 00:14 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461199.66992943:
17:26:44.31 -35:14:45.6 JWST
14:29:42.89 +57:31:51.3 Chandra
18:34:23.06 -24:27:07.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 8 00:14 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461199.66992943 -observatory V36
18:43:31.68 -32:39:08.0 13.6mag P/2010 H2 (Vales)
05:53:26.80 -68:03:51.5 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:49:03.01 +31:58:03.8 17.5mag C/2017 K2 (PANSTARRS)
17:14:44.54 +15:21:02.6 17.8mag C/2021 G2 (ATLAS)
21:12:03.39 -49:30:01.6 16.9mag P/2021 N1 (ZTF)
23:12:38.35 +31:35:28.0 17.2mag C/2022 E2 (ATLAS)
05:34:00.72 +26:58:31.4 16.5mag C/2022 N2 (PANSTARRS)
09:29:42.61 +31:05:00.7 16.6mag C/2022 QE78 (ATLAS)
08:50:31.97 +03:55:50.8 17.7mag C/2022 R6 (PANSTARRS)
18:28:14.31 +21:36:06.8 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:19:22.93 -11:00:31.0 17.6mag P/2023 B1 (PANSTARRS)
22:14:26.42 +66:31:37.5 17.7mag C/2023 H5 (Lemmon)
17:46:26.91 -06:41:12.6 13.7mag C/2023 R1 (PANSTARRS)
13:18:06.58 +82:59:56.4 17.9mag C/2023 X2 (Lemmon)
07:10:22.81 +64:18:29.8 17.7mag C/2024 A1 (ATLAS)
06:47:14.02 +27:49:55.7 13.6mag C/2024 E1 (Wierzchos)
15:37:18.51 +13:31:27.4 17.4mag C/2024 G6 (ATLAS)
20:13:03.75 +31:07:41.0 14.0mag C/2024 J3 (ATLAS)
04:18:00.07 -15:57:11.5 16.0mag C/2024 T5 (ATLAS)
06:05:53.29 +34:29:45.0 17.9mag C/2025 J1 (Borisov)
11:34:55.05 +52:45:02.0 17.4mag C/2025 L1 (ATLAS)
06:44:54.74 -10:52:07.2 14.1mag C/2025 R3 (PANSTARRS)
09:24:08.49 +23:20:25.3 17.9mag C/2025 V2 (Rankin)
12:39:42.12 +04:41:28.2 17.2mag C/2025 Y1 (ATLAS)
18:12:55.60 +75:07:37.3 17.9mag C/2026 A2 (Bok)
02:00:37.33 +43:24:48.7 16.1mag C/2026 B2 (Sun-Gao)
11:11:18.44 -03:44:31.2 16.5mag A/2026 E1
20:23:36.35 -08:34:03.9 8.7mag 10P/Tempel
11:01:59.97 -00:58:03.5 16.0mag 29P/Schwassmann-Wachmann
03:11:40.94 +25:38:32.7 17.7mag 47P/Ashbrook-Jackson
08:59:55.63 +23:46:34.4 16.9mag 63P/Wild
00:26:54.35 -06:22:08.6 15.7mag 65P/Gunn
06:43:21.58 +33:25:39.3 16.9mag 76P/West-Kohoutek-Ikemura
03:09:07.26 +17:12:48.7 13.8mag 78P/Gehrels
01:20:42.29 +04:50:38.3 15.6mag 88P/Howell
04:54:33.63 +30:18:04.4 15.2mag 93P/Lovas
02:42:52.81 +27:37:19.7 17.6mag 114P/Wiseman-Skiff
06:50:29.30 +33:02:20.9 15.6mag 123P/West-Hartley
09:50:08.16 +14:38:53.2 16.5mag 124P/Mrkos
03:58:59.66 +19:14:55.8 16.4mag 128P/Shoemaker-Holt
04:33:30.84 +19:05:00.2 17.7mag 131P/Mueller
05:58:12.29 +18:40:05.7 14.6mag 141P/Machholz
06:00:50.45 +17:40:26.5 14.6mag 141P-A/Machholz
04:53:57.92 +16:10:13.2 11.6mag 141P-D/Machholz
02:57:39.62 -24:42:10.8 16.8mag 161P/Hartley-IRAS
03:41:27.92 +23:47:58.9 14.9mag 162P/SidingSpring
19:36:38.26 +01:43:19.2 16.9mag 169P/NEAT
00:18:16.14 +02:27:37.9 17.9mag 220P/McNaught
16:52:12.16 -08:28:37.2 16.4mag 235P/LINEAR
07:34:36.05 +35:29:34.8 17.5mag 240P/NEAT
00:32:17.12 -02:28:46.5 16.4mag 260P/McNaught
04:04:09.41 +32:28:35.6 17.6mag 295P/LINEAR
23:52:05.60 -09:44:31.0 17.6mag 320P/McNaught
15:15:14.98 +08:06:02.4 17.4mag 391P/Kowalski
08:07:07.02 +20:44:53.0 17.9mag 450P/LONEOS
06:59:55.92 +41:41:53.9 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.7K Jun 8 00:14 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
-rw-r--r-- 1 apache apache 189K Jun 8 00:14 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:39:35.110 +15:17:58.28 AT 2026nsc 2026-05-09.80 20.76
16:42:48.680 +20:27:18.30 AT 2026nsb 2026-05-09.80 20.54
13:34:03.440 +31:37:31.73 AT 2026nsa 2026-05-07.80 21.26
13:50:28.150 +02:34:54.72 AT 2026nrz 2026-05-22.72 21.54
13:43:59.750 +03:47:21.63 AT 2026nry 2026-05-22.69 22.05
13:17:26.150 -01:26:00.12 AT 2026nrx 2026-05-21.64 21.7
00:35:20.216 -08:28:38.64 AT 2026nrw 2026-05-19.42 18.74
23:50:43.016 -01:09:12.25 AT 2026nrv 2026-05-23.48 19.5028
22:36:47.715 +37:31:34.81 AT 2026nru 2026-05-22.43 19.4626
23:58:04.247 +20:56:44.66 AT 2026nrt 2026-05-23.48 20.1237
16:08:58.229 +36:53:23.76 AT 2026nrs 2026-05-21.36 20.3819
19:44:04.734 +84:44:44.91 SN 2026nrr 2026-05-25.47 17.808
21:42:24.388 -20:21:08.51 SN 2026nrq 2026-05-25.56 18.623
22:03:20.669 -84:55:27.45 AT 2026nrp 2026-05-22.30 19.244
23:07:53.376 -39:04:26.84 AT 2026nro 2026-05-22.38 19.567
00:40:07.848 -39:10:21.32 AT 2026nrn 2026-05-12.41 18.737
23:05:28.381 -21:25:50.28 AT 2026nrm 2026-05-25.58 18.887
19:27:28.750 -48:42:52.35 AT 2026nrl 2026-05-22.24 19.107
12:33:38.422 +12:02:05.88 AT 2026nrk 2026-05-25.29 21.322
12:32:27.199 +02:39:54.51 AT 2026nrj 2026-05-25.29 21.0728
-rw-r--r-- 1 apache apache 30K Jun 8 00:14 tns_transients_list.txt
