Design and performance of the GAMMA-400 gamma-ray telescope for dark matter searches. AIP Conference Proceedings Volume 1516, 2013, Pages 288-292

14 сентября 2018
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Контактные данные автора публикации Galper, A.M.ab, Adriani, O.c, Aptekar, R.L.d, Arkhangelskaja, I.V.b, Arkhangelskiy, A.I.b, Boezio, M.e, Bonvicini, V.e
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The GAMMA-400 gamma-ray telescope is designed to measure the fluxes of gamma-rays and cosmic-ray electrons positrons, which can be produced by annihilation or decay of the dark matter particles, as well as to survey the celestial sphere in order to study point and extended sources of gamma-rays, measure energy spectra of Galactic and extragalactic diffuse gamma-ray emission, gamma-ray bursts, and gamma-ray emission from the Sun. GAMMA-400 covers the energy range from 100 MeV to 3000 GeV. Its angular resolution is ∼0.01° (Eγ > 100 GeV), the energy resolution ∼1% (E γ > 10 GeV), and the proton rejection factor ∼10 6. GAMMA-400 will be installed on the Russian space platform Navigator. The beginning of observations is planned for 2018. © 2013 American Institute of Physics.


Author keywords

cosmic gamma-ray emission; dark matter; gamma-ray telescope
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