VERITAS Measurements Of TeV Gamma-Ray Emission From The Supernova Remnant IC 443

Details VERITAS Measurements Of TeV Gamma-Ray Emission From The Supernova Remnant IC 443 VERITAS Measurements Of TeV Gamma-Ray Emission From The Supernova Remnant IC 443

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21110021k&link_type=abstract

American Astronomical Society, AAS Meeting #211, #100.21; Bulletin of the American Astronomical Society, Vol. 39, p.915

Astronomy and Astrophysics

Astronomy

Scientific paper

VERITAS is an array of four 12-m telescopes dedicated to
gamma-ray astronomy in the energy band above 100 GeV. Located near Mt. Hopkins in southern Arizona, VERITAS operated during the 2006-2007 season in 2-, 3-, and 4-telescope observation modes. VERITAS observed IC 443 during 2007, resulting in a strong detection of VHE gamma-ray emission. IC 443 is a shell-type SNR interacting with a molecular cloud and containing a pulsar wind nebula.
In this talk, results from these observations will be discussed in the context of existing multiwavelength data on IC 443.

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