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The GAMMA-400 experiment : Status and prospects

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)
Bergstrom, L. (author)
Berti, E. (author)
Bigongiari, G. (author)
Bobkov, S. G. (author)
Bogomolov, E. A. (author)
Boezio, M. (author)
Bongi, M. (author)
Bonechi, S. (author)
Bottai, S. (author)
Boyarchuk, K. A. (author)
Vacchi, A. (author)
Vannuccini, E. (author)
Vasilyev, G. I. (author)
Castellini, G. (author)
Cattaneo, P. W. (author)
Cumani, P. (author)
Dedenko, G. L. (author)
Dogiel, V. A. (author)
De Donato, C. (author)
Hnatyk, B. I. (author)
Gorbunov, M. S. (author)
Gusakov, Y. V. (author)
Zampa, N. (author)
Zverev, V. G. (author)
Zirakashvili, V. N. (author)
Kadilin, V. V. (author)
Kaplin, V. A. (author)
Kaplun, A. A. (author)
Korepanov, V. E. (author)
Larsson, Josefin (author)
KTH,Partikel- och astropartikelfysik
Leonov, A. A. (author)
Loginov, V. A. (author)
Longo, F. (author)
Maestro, P. (author)
Marrocchesi, P. S. (author)
Mikhailov, V. V. (author)
Mocchiutti, E. (author)
Moiseev, A. A. (author)
Mori, N. (author)
Moskalenko, I. V. (author)
Naumov, P. Y. (author)
Papini, P. (author)
Picozza, P. (author)
Pearce, Mark, 1970- (author)
KTH,Partikel- och astropartikelfysik
Popov, A. V. (author)
Ryde, Felix (author)
KTH,Partikel- och astropartikelfysik
Rappoldi, A. (author)
Ricciarini, S. (author)
Runtso, M. F. (author)
Serdin, O. V. (author)
Sparvoli, R. (author)
Spillantini, P. (author)
Suchkov, S. I. (author)
Tavani, M. (author)
Taraskin, A. A. (author)
Tiberio, A. (author)
Tyurin, E. M. (author)
Ulanov, M. V. (author)
Fuglesang, Christer (author)
KTH,Partikel- och astropartikelfysik
Kheymits, M. D. (author)
Yurkin, Y. T. (author)
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 (creator_code:org_t)
2015
2015
English.
In: Bulletin of the Russian Academy of Sciences: Physics. - 1062-8738. ; 79:3, s. 417-420
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • 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.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Publication and Content Type

ref (subject category)
art (subject category)

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