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The GAMMA-400 experiment: Status and prospects
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2015 (English)In: Bulletin of the Russian Academy of Sciences: Physics, ISSN 1062-8738, Vol. 79, no 3, 417-420 p.Article in journal (Refereed) Published
Abstract [en]

The development of the GAMMA-400 γ-ray telescope continues. The GAMMA-400 is designed to measure fluxes of γ-rays and the electron-positron cosmic-ray component possibly associated with annihilation or decay of dark matter particles; and to search for and study in detail discrete γ-ray sources, to measure the energy spectra of Galactic and extragalactic diffuse γ-rays, and to study γ-ray bursts and γ-rays from the active Sun. The energy range for measuring γ-rays and electrons (positrons) is from 100 MeV to 3000 GeV. For 100-GeV γ-rays, the γ-ray telescope has an angular resolution of ∼0.01°, an energy resolution of ∼1%, and a proton rejection factor of ∼5 × 105. The GAMMA-400 will be installed onboard the Russian Space Observatory.

Place, publisher, year, edition, pages
2015. Vol. 79, no 3, 417-420 p.
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Astronomy, Astrophysics and Cosmology
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URN: urn:nbn:se:kth:diva-167000DOI: 10.3103/S1062873815030429Scopus ID: 2-s2.0-84928111559OAI: oai:DiVA.org:kth-167000DiVA: diva2:818717
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QC 20150609

Available from: 2015-06-09 Created: 2015-05-21 Last updated: 2015-06-09Bibliographically approved

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Larsson, JosefinPearce, MarkRyde, FelixFuglesang, Christer

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