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 GAMMA-400 energy range is expected to be from ∼20 MeV up to TeV energies for gamma rays, up to 10 TeV for electrons + positrons, and up to 1015 eV for cosmic-ray nuclei. For 100-GeV gamma rays, the GAMMA-400 angular resolution is ∼0.01° and energy resolution is ∼1%; the proton rejection factor is ∼5x105. GAMMA-400 will be installed onboard the Russian space observatory.

Details

Title
The GAMMA-400 gamma-ray telescope for precision gamma-ray emission investigations
Author
Topchiev, N P 1 ; Galper, A M 2 ; Bonvicini, V 3 ; Adriani, O 4 ; Aptekar, R L 5 ; Arkhangelskaja, I V 6 ; Arkhangelskiy, A I 6 ; Bakaldin, A V 6 ; Bergstrom, L 7 ; Berti, E 4 ; Bigongiari, G 8 ; Bobkov, S G 9 ; Boezio, M 3 ; Bogomolov, E A 5 ; Bonechi, L 8 ; Bongi, M 4 ; Bottai, S 4 ; Castellini, G 10 ; Cattaneo, P W 11 ; Cumani, P 12 ; Dalkarov, O D 1 ; Dedenko, G L 6 ; De Donato, C 13 ; Dogiel, V A 1 ; Finetti, N 4 ; Gascon, D 14 ; Gorbunov, M S 9 ; Gusakov, Yu V 1 ; Hnatyk, B I 15 ; Kadilin, V V 6 ; Kaplin, V A 6 ; Kaplun, A A 6 ; Kheymits, M D 6 ; Korepanov, V E 16 ; Larsson, J 17 ; Leonov, A A 2 ; Loginov, V A 6 ; Longo, F 3 ; Maestro, P 8 ; Marrocchesi, P S 8 ; Martinez, M 18 ; Men'shenin, A L 19 ; Mikhailov, V V 6 ; Mocchiutti, E 3 ; Moiseev, A A 20 ; Mori, N 4 ; Moskalenko, I V 21 ; P Yu Naumov 6 ; Papini, P 4 ; Paredes, J M 14 ; Pearce, M 17 ; Picozza, P 13 ; Rappoldi, A 11 ; Ricciarini, S 10 ; Runtso, M F 6 ; Ryde, F 17 ; Serdin, O V 9 ; Sparvoli, R 13 ; Spillantini, P 4 ; Stozhkov, Yu I 1 ; Suchkov, S I 1 ; Taraskin, A A 6 ; Tavani, M 22 ; Tiberio, A 4 ; Tyurin, E M 6 ; Ulanov, M V 5 ; Vacchi, A 3 ; Vannuccini, E 4 ; Vasilyev, G I 5 ; Ward, J E 18 ; Yurkin, Yu T 6 ; Zampa, N 3 ; Zirakashvili, V N 23 ; Zverev, V G 6 

 Lebedev Physical Institute, RU-119991 Moscow, Russia 
 Lebedev Physical Institute, RU-119991 Moscow, Russia; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Kashirskoe highway 31, Moscow, 115409, Russia 
 Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I-34149 Trieste, Italy 
 Istituto Nazionale di Fisica Nucleare, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy 
 Ioffe Physical Technical Institute, RU-194021 St. Petersburg, Russia 
 National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Kashirskoe highway 31, Moscow, 115409, Russia 
 The Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova University Center, SE-106 91, Stockholm, Sweden 
 Department of Physical Sciences, Earth and Environment, University of Siena and Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Italy 
 Scientific Research Institute for System Analysis, RU-117218, Moscow, Russia 
10  Istituto di Fisica Applicata Nello Carrara, I-50019, Sesto Fiorentino, Florence, Italy 
11  Istituto Nazionale di Fisica Nucleare, Sezione di Pavia, I-27100, Pavia, Italy 
12  Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I-34149 Trieste, Italy; Institut de Fisica d'Altes Energies, Bellaterra, Spain 
13  Istituto Nazionale di Fisica Nucleare, Sezione di Rome “Tor Vergata”, I-00133, Rome, Italy 
14  Departament d'Astronomia i Meteorologia, Institut de Ciències del Cosmos, Universitat de Barcelona, Spain 
15  Taras Shevchenko National University, Kyiv, 01601, Ukraine 
16  Lviv Center of Institute of Space Research, Lviv, 79060, Ukraine 
17  KTH Royal Institute of Technology, Department of Physics and the Oskar Klein Centre, AlbaNova University Center, SE-10691, Stockholm, Sweden 
18  Institut de Fisica d'Altes Energies, Bellaterra, Spain 
19  Research Institute for Electromechanics, RU-143502 Istra, Moscow region, Russia 
20  NASA Goddard Space Flight Center and CRESST/University of Maryland, Greenbelt, Maryland 20771, USA 
21  Hansen Experimental Physics Laboratory and Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA, 94305, USA 
22  Istituto Nazionale di Astrofisica IASF and Physics Department of University of Rome Tor Vergata, I-00133, Roma, Italy 
23  Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, Troitsk, Moscow region, Russia 
Publication year
2016
Publication date
Feb 2016
Publisher
IOP Publishing
ISSN
17426588
e-ISSN
17426596
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2574999456
Copyright
© 2016. This work is published under http://creativecommons.org/licenses/by/3.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.