VERITAS Observation of the E>200GeV Gamma-ray Sky

Details VERITAS Observation of the E>200GeV Gamma-ray Sky VERITAS Observation of the E>200GeV Gamma-ray Sky

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21430205l&link_type=abstract

American Astronomical Society, AAS Meeting #214, #302.05; Bulletin of the American Astronomical Society, Vol. 41, p.719

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VERITAS is an array of four 12-m diameter imaging atmospheric Cherekov telescopes located in southern Arizona. The array has been in full operation since Fall 2007 and is sensitive to very high energy gamma-rays above 100 GeV. VERITAS has been used to detect new sources of TeV emission, such as the blazars 1ES 0806+524, RGB J0710+591 and W Comae, and to study many other source classes including supernova remnants, gamma-ray binaries and radio galaxies. We will present a review of recent VERITAS results.

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