The EVLA: A New Mission for High Energy Astrophysics

Details The EVLA: A New Mission for High Energy Astrophysics The EVLA: A New Mission for High Energy Astrophysics

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010head...11.4807f&link_type=abstract

American Astronomical Society, HEAD meeting #11, #48.07; Bulletin of the American Astronomical Society, Vol. 41, p.740

Astronomy and Astrophysics

Astrophysics

Scientific paper

Beginning March 2010 the Very Large Array (VLA) will be replaced by a new telescope, the Expanded VLA (EVLA). When it is fully complete in 2012 the EVLA will have a continuum sensitivity improvement over the VLA by factors of 5 to 20. It will also have complete frequency coverage from 1 to 50 GHz and enormously improved spectral capability.
The EVLA will be able to address a broad range of problems in high energy astrophysics including X-ray binaries, galactic black holes, supernovae, gamma-ray bursts, active galactic nuclei, clusters and the intercluster medium. I will show by example how the capabilities of the EVLA will be used to address some of these problems.

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