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GAMMA-400 gamma-ray observatory

Topchiev, N. P. (author)
Galper, A. M. (author)
Bonvicini, V. (author)
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Adriani, O. (author)
Aptekar, R. L. (author)
Arkhangelskaja, I. V. (author)
Arkhangelskiy, A. I. (author)
Bakaldin, A. V. (author)
Bergstrom, L. (author)
Berti, E. (author)
Bigongiari, G. (author)
Bobkov, S. G. (author)
Boezio, M. (author)
Bogomolov, E. A. (author)
Bonechi, L. (author)
Bongi, M. (author)
Bottai, S. (author)
Castellini, G. (author)
Cattaneo, P. W. (author)
Cumani, P. (author)
Dalkarov, O. D. (author)
Dedenko, G. L. (author)
DeDonato, C. (author)
Dogiel, V. A. (author)
Finetti, N. (author)
Gascon, D. (author)
Gorbunov, M. S. (author)
Gusakov, Yu.V. (author)
Hnatyk, B. I. (author)
Kadilin, V. V. (author)
Kaplin, V. A. (author)
Kaplun, A. A. (author)
Kheymits, M. D. (author)
Korepanov, V. E. (author)
Larsson, J. (author)
Leonov, A. A. (author)
Loginov, V. A. (author)
Longo, F. (author)
Maestro, P. (author)
Marrocchesi, P. S. (author)
Martinez, M. (author)
Men'Shenin, A. L. (author)
Mikhailov, V. V. (author)
Mocchiutti, E. (author)
Moiseev, A. A. (author)
Mori, N. (author)
Moskalenko, I. V. (author)
Naumov, P.Yu. (author)
Papini, P. (author)
Paredes, J. M. (author)
Pearce, Mark (author)
KTH,Partikel- och astropartikelfysik,Oskar Klein Centre, AlbaNova University Center
Picozza, P. (author)
Rappoldi, A. (author)
Ricciarini, S. (author)
Runtso, M. F. (author)
Ryde, Felix (author)
KTH,Partikel- och astropartikelfysik,Oskar Klein Centre, AlbaNova University Center
Serdin, O. V. (author)
Sparvoli, R. (author)
Spillantini, P. (author)
Stozhkov, Yu.I. (author)
Suchkov, S. I. (author)
Taraskin, A. A. (author)
Tavani, M. (author)
Tiberio, A. (author)
Tyurin, E. M. (author)
Ulanov, M. V. (author)
Vacchi, A. (author)
Vannuccini, E. (author)
Vasilyev, G. I. (author)
Ward, J. E. (author)
Yurkin, Yu.T. (author)
Zampa, N. (author)
Zirakashvili, V. N. (author)
Zverev, V. G. (author)
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 (creator_code:org_t)
Proceedings of Science (PoS), 2015
2015
English.
In: Proceedings of Science. - : Proceedings of Science (PoS).
  • Conference paper (peer-reviewed)
Abstract Subject headings
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  • 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 fromGalactic Center, Crab, Vela, Cygnus, Geminga, and other regions will be performed, as well asdiffuse gamma-rayemission,along with measurements of high-energy electron + positron and nuclei fluxes. Furthermore, it will studygamma-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 10 TeV for electrons + positrons, and up to 1015eV 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° to ∼0.01° and energy resolution from 3% to ∼1%; the proton rejection factor is ∼5x105. GAMMA-400 will be installed onboardthe Russian space observatory.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Publication and Content Type

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