Joint Astrophysics Colloquium
Astronomy at photon energies beyond 100 GeV � Recent
results from VERITAS
Gernot Maier
McGill
VERITAS (Very Energetic Radiation Imaging Telescope Array System) is a major
observatory for gamma-ray astronomy in the 100 GeV-50 TeV energy band. The
observatory, located on Mt. Hopkins, AZ, consists of four 12 m-diameter
telescopes that detect very high-energy gamma rays via the imaging atmospheric
Cherenkov technique. VERITAS became fully operational in Spring 2007 and
has embarked on a broad program of observations of galactic and extragalactic
sources. I will summarize the major results from the observatory, concentrating
on observations of X-ray binaries and extragalactic blazars.
Tuesday, January 20th 2009, 16:00
Ernest Rutherford Physics Building, R.E. Bell Conference Room (room 103)
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