Radio Observations of SN2004gk

Details Radio Observations of SN2004gk Radio Observations of SN2004gk

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..351....1s&link_type=abstract

The Astronomer's Telegram, #351

Astronomy and Astrophysics

Astronomy

1

Radio, Nova, Supernova

Scientific paper

We observed the Type Ic SN2004gk (IAUC #8446) with the Very Large Array at 8.5 GHz on 2004 Nov 30.57 UT. We do not detect radio emission from the supernova and place a 2-sigma limit of 0.10 mJy at the optical position. Assuming a distance of 15 Mpc to the SN host galaxy (IC 3311), this VLA observation implies an upper limit on the SN2004gk radio luminosity of ~ 10^25 erg/s/Hz, making it four orders of magnitude less radio luminous than SN1998bw and comparable to SN2002ap at a similar epoch.

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