Simulation based evaluation of the designs of the Advanced Gamma-ray Imageing System (AGIS)
POSTER
Abstract
The AGIS project under design study, is a large array of imaging atmospheric Cherenkov telescopes for gamma-rays astronomy between 40GeV and 100 TeV. In this paper we present the ongoing simulation effort to model the considered design approaches as a function of the main parameters such as array geometry, telescope optics and camera design in such a way the gamma ray observation capabilities can be optimized against the overall project cost.
Authors
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Slava Bugaev
Washington University in St. Louis
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James Buckley
Washington University, Washington University in St. Louis
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Seth Digel
SLAC, Stanford/SLAC Kavli Institute for Particle Astrophysics
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Stephen Funk
Stanford/SLAC Kavli Institute for Particle Astrophysics
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Alex Konopelko
Pittsburg State University
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Henric Krawczynski
Washington University
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Stephan Le Bohec
University of Utah
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Gernot Maier
McGill University
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Vladimir Vassiliev
UCLA