2011CBET.2946....4R

Query : 2011CBET.2946....4R

2011CBET.2946....4R - Central Bureau Electronic Telegrams, 2946, 4 (2011/December-0)

Supernova 2011ja in NGC 4945 = PSN J13051112-4931270.

RYDER S., SODERBERG A., STOCKDALE C., VAN DYK S., IMMLER S., WEILER K. and PANAGIA N.

Abstract (from CDS):

S. Ryder, Australian Astronomical Observatory; A. Soderberg, Harvard University; C. Stockdale, Marquette University; S. Van Dyk, Spitzer Science Center, California Institute of Technology; S. Immler, Goddard Space Flight Center; K. Weiler, Naval Research Laboratory; and N. Panagia, Space Telescope Science Institute and Observatory of Catania, report the detection of radio emission near the position of SN 2011ja with the Australia Telescope Compact Array radio telescope, confirming its core-collapse nature. A flux density of 0.44 ± 0.20 mJy was measured at 18.0 GHz on Dec 19.9 UT. The measured position of the radio emission of R.A. = 13:05:11.06, Decl. = -49:31:26.0 (equinox 2000.0) is in good agreement with the measured optical position (end figures 11s.12, 27".0). Radio observations of this nearby (4 Mpc, from NED) supernova at the Australia Telescope Compact Array are continuing.

Abstract Copyright: ∼

Journal keyword(s):

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 SN 2011ja SN* 13 05 11.12 -49 31 27.0           SNIIP 48 0

Query : 2011CBET.2946....4R

Basic data :
SN 2011ja -- SuperNova
Other object types: otypes_help 		SN* (SN), SN? (PSN)
ICRS coord. (ep=J2000) : 		13 05 11.12 -49 31 27.0 [ ] B 2011CBET.2946....1M
FK4 coord. (ep=B1950 eq=1950) : 		13 02 15.97 -49 15 23.0 [ ]
Gal coord. (ep=J2000) : 		305.22348 +13.28640 [ ]
Spectral type: 		SNIIP C 2015MNRAS.452.2597X
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Identifiers (2) :
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SN 2011ja PSN J13051112-4931270

References (48 between 1850 and 2026) (Total 48)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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