Next generation of IACT arrays: scientific objectives versus energy domains

Details Next generation of IACT arrays: scientific objectives versus energy domains Next generation of IACT arrays: scientific objectives versus energy domains

2005-11-04

arxiv.org/abs/astro-ph/0511139v1

Astronomy and Astrophysics

Astrophysics

14 pages, Invited talk at the Conference "Towards a Network of Atmospheric Cherenkov Detectors VII", 2005, Palaiseau, France

Scientific paper

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 \textit{multi-GeV} ($E \leq$ 30 GeV), low or \textit{sub-TeV} (30 GeV - 300 GeV), high or \textit{TeV} (300 GeV - 30 TeV), and very-high or \textit{sub-PeV} ($E \geq$ 30 TeV) intervals -- to be covered by the next generation of IACT arrays.

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