author_facet Topchiev, N.P.
Galper, A.M.
Arkhangelskaja, I.V.
Arkhangelskiy, A.I.
Bakaldin, A.V.
Chernysheva, I.V.
Dalkarov, O.D.
Egorov, A.E.
Gusakov, Yu.V.
Kheymits, M.D.
Leonov, A.A.
Naumov, P.Yu.
Pappe, N.Yu.
Runtso, M.F.
Stozhkov, Yu.I.
Suchkov, S.I.
Yurkin, Yu.T.
Zverev, V.G.
Topchiev, N.P.
Galper, A.M.
Arkhangelskaja, I.V.
Arkhangelskiy, A.I.
Bakaldin, A.V.
Chernysheva, I.V.
Dalkarov, O.D.
Egorov, A.E.
Gusakov, Yu.V.
Kheymits, M.D.
Leonov, A.A.
Naumov, P.Yu.
Pappe, N.Yu.
Runtso, M.F.
Stozhkov, Yu.I.
Suchkov, S.I.
Yurkin, Yu.T.
Zverev, V.G.
author Topchiev, N.P.
Galper, A.M.
Arkhangelskaja, I.V.
Arkhangelskiy, A.I.
Bakaldin, A.V.
Chernysheva, I.V.
Dalkarov, O.D.
Egorov, A.E.
Gusakov, Yu.V.
Kheymits, M.D.
Leonov, A.A.
Naumov, P.Yu.
Pappe, N.Yu.
Runtso, M.F.
Stozhkov, Yu.I.
Suchkov, S.I.
Yurkin, Yu.T.
Zverev, V.G.
spellingShingle Topchiev, N.P.
Galper, A.M.
Arkhangelskaja, I.V.
Arkhangelskiy, A.I.
Bakaldin, A.V.
Chernysheva, I.V.
Dalkarov, O.D.
Egorov, A.E.
Gusakov, Yu.V.
Kheymits, M.D.
Leonov, A.A.
Naumov, P.Yu.
Pappe, N.Yu.
Runtso, M.F.
Stozhkov, Yu.I.
Suchkov, S.I.
Yurkin, Yu.T.
Zverev, V.G.
EPJ Web of Conferences
High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
General Earth and Planetary Sciences
General Engineering
General Environmental Science
author_sort topchiev, n.p.
spelling Topchiev, N.P. Galper, A.M. Arkhangelskaja, I.V. Arkhangelskiy, A.I. Bakaldin, A.V. Chernysheva, I.V. Dalkarov, O.D. Egorov, A.E. Gusakov, Yu.V. Kheymits, M.D. Leonov, A.A. Naumov, P.Yu. Pappe, N.Yu. Runtso, M.F. Stozhkov, Yu.I. Suchkov, S.I. Yurkin, Yu.T. Zverev, V.G. 2100-014X EDP Sciences General Earth and Planetary Sciences General Engineering General Environmental Science http://dx.doi.org/10.1051/epjconf/201920814004 <jats:p>The 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 ~ 20 MeV to several TeV and electron + positron fluxes up 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 (~ 0.01° at E<jats:sub>γ</jats:sub> = 100 GeV) and energy (~ 1% at E<jats:sub>γ</jats:sub> = 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.</jats:p> High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope EPJ Web of Conferences
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title High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
title_unstemmed High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
title_full High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
title_fullStr High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
title_full_unstemmed High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
title_short High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
title_sort high-energy gamma- and cosmic-ray observations with future space-based gamma-400 gamma-ray telescope
topic General Earth and Planetary Sciences
General Engineering
General Environmental Science
url http://dx.doi.org/10.1051/epjconf/201920814004
publishDate 2019
physical 14004
description <jats:p>The 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 ~ 20 MeV to several TeV and electron + positron fluxes up 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 (~ 0.01° at E<jats:sub>γ</jats:sub> = 100 GeV) and energy (~ 1% at E<jats:sub>γ</jats:sub> = 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.</jats:p>
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author Topchiev, N.P., Galper, A.M., Arkhangelskaja, I.V., Arkhangelskiy, A.I., Bakaldin, A.V., Chernysheva, I.V., Dalkarov, O.D., Egorov, A.E., Gusakov, Yu.V., Kheymits, M.D., Leonov, A.A., Naumov, P.Yu., Pappe, N.Yu., Runtso, M.F., Stozhkov, Yu.I., Suchkov, S.I., Yurkin, Yu.T., Zverev, V.G.
author_facet Topchiev, N.P., Galper, A.M., Arkhangelskaja, I.V., Arkhangelskiy, A.I., Bakaldin, A.V., Chernysheva, I.V., Dalkarov, O.D., Egorov, A.E., Gusakov, Yu.V., Kheymits, M.D., Leonov, A.A., Naumov, P.Yu., Pappe, N.Yu., Runtso, M.F., Stozhkov, Yu.I., Suchkov, S.I., Yurkin, Yu.T., Zverev, V.G., Topchiev, N.P., Galper, A.M., Arkhangelskaja, I.V., Arkhangelskiy, A.I., Bakaldin, A.V., Chernysheva, I.V., Dalkarov, O.D., Egorov, A.E., Gusakov, Yu.V., Kheymits, M.D., Leonov, A.A., Naumov, P.Yu., Pappe, N.Yu., Runtso, M.F., Stozhkov, Yu.I., Suchkov, S.I., Yurkin, Yu.T., Zverev, V.G.
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container_title EPJ Web of Conferences
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description <jats:p>The 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 ~ 20 MeV to several TeV and electron + positron fluxes up 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 (~ 0.01° at E<jats:sub>γ</jats:sub> = 100 GeV) and energy (~ 1% at E<jats:sub>γ</jats:sub> = 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.</jats:p>
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spelling Topchiev, N.P. Galper, A.M. Arkhangelskaja, I.V. Arkhangelskiy, A.I. Bakaldin, A.V. Chernysheva, I.V. Dalkarov, O.D. Egorov, A.E. Gusakov, Yu.V. Kheymits, M.D. Leonov, A.A. Naumov, P.Yu. Pappe, N.Yu. Runtso, M.F. Stozhkov, Yu.I. Suchkov, S.I. Yurkin, Yu.T. Zverev, V.G. 2100-014X EDP Sciences General Earth and Planetary Sciences General Engineering General Environmental Science http://dx.doi.org/10.1051/epjconf/201920814004 <jats:p>The 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 ~ 20 MeV to several TeV and electron + positron fluxes up 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 (~ 0.01° at E<jats:sub>γ</jats:sub> = 100 GeV) and energy (~ 1% at E<jats:sub>γ</jats:sub> = 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.</jats:p> High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope EPJ Web of Conferences
spellingShingle Topchiev, N.P., Galper, A.M., Arkhangelskaja, I.V., Arkhangelskiy, A.I., Bakaldin, A.V., Chernysheva, I.V., Dalkarov, O.D., Egorov, A.E., Gusakov, Yu.V., Kheymits, M.D., Leonov, A.A., Naumov, P.Yu., Pappe, N.Yu., Runtso, M.F., Stozhkov, Yu.I., Suchkov, S.I., Yurkin, Yu.T., Zverev, V.G., EPJ Web of Conferences, High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope, General Earth and Planetary Sciences, General Engineering, General Environmental Science
title High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
title_full High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
title_fullStr High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
title_full_unstemmed High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
title_short High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
title_sort high-energy gamma- and cosmic-ray observations with future space-based gamma-400 gamma-ray telescope
title_unstemmed High-energy gamma- and cosmic-ray observations with future space-based GAMMA-400 gamma-ray telescope
topic General Earth and Planetary Sciences, General Engineering, General Environmental Science
url http://dx.doi.org/10.1051/epjconf/201920814004