EVLA Detection of PTF11eon/SN2011dh

Details EVLA Detection of PTF11eon/SN2011dh EVLA Detection of PTF11eon/SN2011dh

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3411....1h&link_type=abstract

The Astronomer's Telegram, #3411

Astronomy and Astrophysics

Astronomy

3

Radio, Supernovae

Scientific paper

We triggered our NRAO Target Of Opportunity programs (PI Kasliwal; PI Stockdale) and used the Expanded Very Large Array (EVLA) to observe PTF11eon/SN2011dh (ATEL#3398), a very young Type II supernova. EVLA observations were undertaken on 2011 June 04.25 UT. We detect radio emission at a center frequency of 22.46 GHz (K band) at a flux of 2.68 ± 0.10 mJy/beam. The spectral luminosity density is therefore 2.02+/-0.08 1026 erg s-1 Hz-1.

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