EVLA and Swift Follow Up of PTF10abyy

Details EVLA and Swift Follow Up of PTF10abyy EVLA and Swift Follow Up of PTF10abyy

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.3093....1k&link_type=abstract

The Astronomer's Telegram, #3093

Astronomy and Astrophysics

Astronomy

Radio, Ultra-Violet, X-Ray, Supernovae, Transient

Scientific paper

We triggered our NRAO Target Of Opportunity program "Exploring Transients in the Local Universe" and used the Expanded Very Large Array (EVLA) to observe PTF10abyy (ATEL#3091), a young Type II supernova discovered by the Palomar Transient Factory. The EVLA observations were made on 2010 December 10.28 UT. We detect no radio emission at a center frequency of 8.46 GHz down to a 3-sigma limit of 81 uJy.

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