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High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope

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dc.contributor.authorTopchiev, N. P.
dc.contributor.authorGalper, A. M.
dc.contributor.authorArkhangelskaja, I. V.
dc.contributor.authorArkhangelskiy, A. I.
dc.contributor.authorChernysheva, I. V.
dc.contributor.authorKheymits, M. D.
dc.contributor.authorLeonov, A. A.
dc.contributor.authorNaumov, P. Y.
dc.contributor.authorRuntso, M. F.
dc.contributor.authorYurkin, Y. T.
dc.contributor.authorАрхангельская, Ирина Владимировна
dc.contributor.authorАрхангельский, Андрей Игоревич
dc.contributor.authorЧернышева, Ирина Вячеславовна
dc.contributor.authorХеймиц, Максим Дмитриевич
dc.contributor.authorЛеонов, Алексей Анатольевич
dc.contributor.authorНаумов, Петр Юрьевич
dc.contributor.authorЮркин, Юрий Тихонович
dc.date.accessioned2024-11-21T18:55:54Z
dc.date.available2024-11-21T18:55:54Z
dc.date.issued2019
dc.description.abstractThe future space-based GAMMA-400 gamma-ray telescope will be installed on the Navigator platform of the Russian Astrophysical Observatory. A highly elliptical orbit will provide observations for 7-10 years of many regions of the celestial sphere continuously for a long time ( 100 days). GAMMA-400 will measure gamma-ray fluxes in the energy range from similar to 20 MeV to several TeV and electron + positron fluxes up to similar to 20 TeV. GAMMA-400 will have an excellent separation of gamma rays from the background of cosmic rays and electrons + positrons from protons and an unprecedented angular (similar to 0.01 degrees at E-gamma = 100 GeV) and energy (similar to 1% at E-gamma = 100 GeV) resolutions better than for Fermi-LAT, as well as ground-based facilities, by a factor of 5-10. Observations of GAMMA-400 will provide new fundamental data on discrete sources and spectra of gamma-ray emission and electrons + positrons, as well as the nature of dark matter.
dc.identifier.citationHigh-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope / Topchiev, NP [et al.] // XX INTERNATIONAL SYMPOSIUM ON VERY HIGH ENERGY COSMIC RAY INTERACTIONS (ISVHECRI 2018). - 2019. - 208. - 10.1051/epjconf/201920814004
dc.identifier.doi10.1051/epjconf/201920814004
dc.identifier.urihttps://www.doi.org/10.1051/epjconf/201920814004
dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000570461200070
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/19590
dc.relation.ispartofXX INTERNATIONAL SYMPOSIUM ON VERY HIGH ENERGY COSMIC RAY INTERACTIONS (ISVHECRI 2018)
dc.titleHigh-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
dc.typeProceedings Paper
dspace.entity.typePublication
oaire.citation.volume208
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