Next generation of IACT arrays: scientific objectives versus energy domains

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dc.creatorAharonian, Felix
dc.date2005-11-04
dc.date.accessioned2026-07-07T06:44:52Z
dc.date.available2026-07-07T06:44:52Z
dc.descriptionSeveral 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.
dc.description14 pages, Invited talk at the Conference "Towards a Network of Atmospheric Cherenkov Detectors VII", 2005, Palaiseau, France
dc.identifierhttps://arxiv.org/abs/astro-ph/0511139
dc.identifierhttp://arxiv.org/abs/astro-ph/0511139
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/102895
dc.subjectAstrophysics
dc.titleNext generation of IACT arrays: scientific objectives versus energy domains
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