Next generation of IACT arrays: scientific objectives versus energy domains
Abstract
Several key motivations and perspectives of ground based gamma-ray astronomy are discussed in the context of the specifics of detection techniques and scientific topics/objectives relevant to four major energy domains -- very-low or multi-GeV (E ≤ 30 GeV), low or sub-TeV (30 GeV - 300 GeV), high or TeV (300 GeV - 30 TeV), and very-high or sub-PeV (E ≥ 30 TeV) intervals -- to be covered by the next generation of IACT arrays.
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