Publication: GAMMA-400 Gamma-Ray Observations in the GeV and TeV Energy Range
| dc.contributor.author | Topchiev, N. P. | |
| dc.contributor.author | Bakaldin, A. V. | |
| dc.contributor.author | Cherniy, R. A. | |
| dc.contributor.author | Dalkarov, O. D. | |
| dc.contributor.author | Galper, A. M. | |
| dc.contributor.author | Arkhangelskaja, I. V. | |
| dc.contributor.author | Arkhangelskiy, A. I. | |
| dc.contributor.author | Chernysheva, I. V. | |
| dc.contributor.author | Kheymits, M. D. | |
| dc.contributor.author | Korotkov, M. G. | |
| dc.contributor.author | Leonov, A. A. | |
| dc.contributor.author | Malinin, A. G. | |
| dc.contributor.author | Mikhailov, V. V. | |
| dc.contributor.author | Runtso, M. F. | |
| dc.contributor.author | Yurkin, Y. T. | |
| dc.contributor.author | Архангельская, Ирина Владимировна | |
| dc.contributor.author | Архангельский, Андрей Игоревич | |
| dc.contributor.author | Чернышева, Ирина Вячеславовна | |
| dc.contributor.author | Хеймиц, Максим Дмитриевич | |
| dc.contributor.author | Коротков, Михаил Геннадиевич | |
| dc.contributor.author | Леонов, Алексей Анатольевич | |
| dc.contributor.author | Малинин, Александр Геннадьевич | |
| dc.contributor.author | Михайлов, Владимир Владимирович | |
| dc.contributor.author | Юркин, Юрий Тихонович | |
| dc.date.accessioned | 2024-11-30T01:14:42Z | |
| dc.date.available | 2024-11-30T01:14:42Z | |
| dc.date.issued | 2021 | |
| dc.description.abstract | © 2021, Pleiades Publishing, Ltd.Abstract: The future space-based GAMMA-400 γ-ray telescope will operate onboard the Russian astrophysical observatory in a highly elliptic orbit during 7 years. Observing γ-ray sources from Galactic plane, γ-ray bursts, γ-ray diffuse emission, γ rays from the Sun, and γ rays from dark matter particles will be performed uninterruptedly for a long time (∼100 days) in point-source mode in contrast to scanning mode for Fermi-LAT and other space- and ground-based instruments. GAMMA-400 will measure γ rays in the energy range from ∼20 MeV to several TeV units, have the unprecedented angular (∼0.01° at Eγ = 100 GeV) and energy (∼2% at Eγ =100 GeV) resolutions better than for Fermi-LAT, as well as ground-based γ-ray facilities, by a factor of 5–10, and perfectly separate γ rays from cosmic-ray background. | |
| dc.format.extent | С. 1053-1058 | |
| dc.identifier.citation | GAMMA-400 Gamma-Ray Observations in the GeV and TeV Energy Range / Topchiev, N.P. [et al.] // Physics of Atomic Nuclei. - 2021. - 84. - № 6. - P. 1053-1058. - 10.1134/S106377882113038X | |
| dc.identifier.doi | 10.1134/S106377882113038X | |
| dc.identifier.uri | https://www.doi.org/10.1134/S106377882113038X | |
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| dc.identifier.uri | https://openrepository.mephi.ru/handle/123456789/25165 | |
| dc.relation.ispartof | Physics of Atomic Nuclei | |
| dc.title | GAMMA-400 Gamma-Ray Observations in the GeV and TeV Energy Range | |
| dc.type | Article | |
| dspace.entity.type | Publication | |
| oaire.citation.issue | 6 | |
| oaire.citation.volume | 84 | |
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