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

  • Slava Bugaev

    Washington University in St. Louis

  • James Buckley

    Washington University, Washington University in St. Louis

  • Seth Digel

    SLAC, Stanford/SLAC Kavli Institute for Particle Astrophysics

  • Stephen Funk

    Stanford/SLAC Kavli Institute for Particle Astrophysics

  • Alex Konopelko

    Pittsburg State University

  • Henric Krawczynski

    Washington University

  • Stephan Le Bohec

    University of Utah

  • Gernot Maier

    McGill University

  • Vladimir Vassiliev

    UCLA