EVLA and Swift Follow Up of PTF10abpr

Details EVLA and Swift Follow Up of PTF10abpr EVLA and Swift Follow Up of PTF10abpr

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.3090....1k&link_type=abstract

The Astronomer's Telegram, #3090

Astronomy and Astrophysics

Astronomy

Radio, Optical, 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 PTF10abpr (ATEL#3089), a Type II supernova at a distance of 20 Mpc. The EVLA observations were made on 2010 December 11.22 UT. We detect no radio emission at a center frequency of 8.46 GHz down to a 3-sigma limit of 81 uJy.
Under our ongoing PTF/Swift program, we began observations of PTF10abpr on December 10.01 UT.

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