EVLA Observations of CSS100217:102913+404220

Details EVLA Observations of CSS100217:102913+404220 EVLA Observations of CSS100217:102913+404220

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2629....1f&link_type=abstract

The Astronomer's Telegram, #2629

Astronomy and Astrophysics

Astronomy

Radio, Agn, Black Holes, Novae, Supernovae, Transients

Scientific paper

We used the Expanded Very Large Array (EVLA) to observe the field of view toward a luminous optical transient CSS100217:102913+404220, discovered by the Catalina Real-time Transient Survey (CRTS) (ATel #2544). The EVLA observations were made on April 29.22 UT and May 14.07 UT. For each epoch we observed the source simultaneously at frequencies of 4495 MHz and 7915 MHz for a total of 35 minutes. We detect point-like radio emission that is spatially coincident with the optical transient (1 sigma=+/-0.2 arcsec).

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