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Monte Carlo design studies for the Cherenkov Telescope Array
The Cherenkov Telescopes Array (CTA) is planned as the future instrument for very-high-energy (VHE) gamma-ray astronomy with a wide energy range of four orders of magnitude and an improvement in sensitivity compared to current instruments of about an order of magnitude. Monte Carlo simulations are a crucial tool in the design of CTA. The ultimate goal of these simulations is to find the most cost-effective solution for given physics goals and thus sensitivity goals or to find, for a given cost,doi:10.1016/j.astropartphys.2012.10.002 fatcat:6stbf3ive5ew3pni5wez3672qq