Optimum spacing between imaging atmospheric Cerenkov telescopes in the future 50 GeV multi-telescope arrays

Details Optimum spacing between imaging atmospheric Cerenkov telescopes in the future 50 GeV multi-telescope arrays Optimum spacing between imaging atmospheric Cerenkov telescopes in the future 50 GeV multi-telescope arrays

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..515..323k&link_type=abstract

GeV-TeV GAMMA RAY ASTROPHYSICS WORKSHOP: Towards a Major Atmospheric Cherenkov Detector VI. AIP Conference Proceedings, Volume

Astronomy and Astrophysics

Astrophysics

X- And Gamma-Ray Telescopes And Instrumentation

Scientific paper

Regarding the optimum design of future low energy (50-100 GeV) arrays of
imaging air Čerenkov telescopes an important issue is a choice of
optimum arrangement (layout) of telescopes within the array. Here we
present the basic results of such studies addressed by use of detailed
Monte Carlo simulations. .

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