RA/DEC (2000)
00:42:29.250 +41:14:00.31
10.621875 +41.233419
Type
Nova
Redshift
-0.0012
Reporting Group
None
Discovering Data Source
None
Discovery Date
2019-01-28 18:02:21.000
TNS AT
Y
Public
Y
Host Name
M31
Discovery Mag
16.9
Filter
Clear-
Reporter/s
George Carey
Spectra
▌AT_2019agt - 2019-02-04 18:35:15 Other / Other (None)z=
▌Show H at z=vexp= km/s
▌Show He at z=vexp= km/s
▌Show He II at z=vexp= km/s
▌Show C II at z=vexp= km/s
▌Show C III at z=vexp= km/s
▌Show C IV at z=vexp= km/s
▌Show N II at z=vexp= km/s
▌Show N III at z=vexp= km/s
▌Show N IV at z=vexp= km/s
▌Show N V at z=vexp= km/s
▌Show O at z=vexp= km/s
▌Show [O I] at z=vexp= km/s
▌Show O II at z=vexp= km/s
▌Show [O II] at z=vexp= km/s
▌Show [O III] at z=vexp= km/s
▌Show O V at z=vexp= km/s
▌Show O VI at z=vexp= km/s
▌Show Na at z=vexp= km/s
▌Show Mg at z=vexp= km/s
▌Show Mg II at z=vexp= km/s
▌Show Si II at z=vexp= km/s
▌Show S II at z=vexp= km/s
▌Show Ca II at z=vexp= km/s
▌Show [Ca II] at z=vexp= km/s
▌Show Fe II at z=vexp= km/s
▌Show Fe III at z=vexp= km/s
▌Show Å at z=vexp= km/s
▌Show Å at z=vexp= km/s
▌Show Å at z=vexp= km/s
▌Show Å at z=vexp= km/s
▌Show Tellurics
▌Show Galaxy lines at z=
▌Show WR-WN at z=vexp= km/s
▌Show WR-WC/O at z=vexp= km/s
Binning factor: (rounded to nearest integer >1)
Mouse hovers at WL: 0 (rest),0 (observed)
Comments
TNS System (WIS)
Sun, 06/23/2019 - 10:45
Object coordinates updated
Object coordinates updated according to AT-report 29888 of Group GaiaAlerts
Previous RA, DEC: 00:42:29.220, +41:14:00.80 (10.62175, +41.233556)
Updated RA, DEC: 00:42:29.250, +41:14:00.31 (10.621875, 41.233419)
George Carey (Bromsgrove Astronomical Society, Member of 'The Astronomer' SN and nova search team, Member of the BAA)
Mon, 01/28/2019 - 20:56
Independent discovery
Nick James obtained an image at about the same time: 2019-01-28 18:06:03
Image attached.
George Carey (Bromsgrove Astronomical Society, Member of 'The Astronomer' SN and nova search team, Member of the BAA)
Mon, 01/28/2019 - 19:26
Discovery image
600 second image, photometry and astrometry using Astrometrica.