Radio Observations of SN2005bf

Astronomy and Astrophysics – Astronomy

Scientific paper

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Radio, Novae, Supernovae

Scientific paper

We report on our monitoring of the Type Ibc supernova SN2005bf (IAUC 8507) with the Very Large Array between 2005 Apr 13 and Oct 6 UT. No radio emission is detected from the SN in any of our observations. At 8.46 GHz we place 2-sigma limits of 0.11 and 0.19 mJy for our first and last epochs (t ~ 20 and 200 days after the explosion), respectively. At a distance of 81 Mpc, these limits imply that SN2005bf was at least a factor of 100 less luminous than radio bright SN1998bw on a comparable timescale.

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