Optimization of large homogeneous air Cherenkov arrays and application to the design of a 1–100 TeV γ-ray observatory

At the time large air Cherenkov arrays are being discussed for future γ-ray observatories, we review the relationship between the targeted capabilities and the main design parameters taking into account construction costs. As an example application, we describe a telescope array optimized for observations between 1 TeV and a few 100 TeV and use detailed simulations to estimate its performances in comparison to science objectives.