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• W1603616092 abstract "The GAMMA-400 gamma-ray telescope with excellent angular and energy resolutions is designed to search for signatures of dark matter in the fluxes of gamma-ray emission and electrons + positrons. Precision investigations of gamma-ray emission from Galactic Center, Crab, Vela, Cygnus, Geminga, and other regions will be performed, as well as diffuse gamma-ray emission, along with measurements of high-energy electron + positron and nuclei fluxes. Furthermore, it will study gamma-ray bursts and gamma-ray emission from the Sun during periods of solar activity. The energy range of GAMMA-400 is expected to be from ~20 MeV up to TeV energies for gamma rays, up to 20 TeV for electrons + positrons, and up to 10E15 eV for cosmic-ray nuclei. For high-energy gamma rays with energy from 10 to 100 GeV, the GAMMA-400 angular resolution improves from 0.1{deg} to ~0.01{deg} and energy resolution from 3% to ~1%; the proton rejection factor is ~5x10E5. GAMMA-400 will be installed onboard the Russian space observatory." @default.
• W1603616092 created "2016-06-24" @default.
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• W1603616092 date "2015-07-22" @default.
• W1603616092 modified "2023-09-26" @default.
• W1603616092 title "GAMMA-400 gamma-ray observatory" @default.
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• W1603616092 doi "https://doi.org/10.48550/arxiv.1507.06246" @default.
• W1603616092 hasPublicationYear "2015" @default.
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