Design and Performance of the GAMMA-400 Gamma-Ray Telescope for the Dark Matter Searches
The GAMMA-400 gamma-ray telescope is designed to measure the fluxes of gamma rays and cosmic-ray electrons + positrons, which can be produced by annihilation or decay of the dark matter particles, as well as to survey the celestial sphere in order to study point and extended sources of gamma rays, m...
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| creator | Galper, A M Adriani, O Aptekar, R L Arkhangelskaja, I V Arkhangelskiy, A I Boezio, M Bonvicini, V Boyarchuk, K A Fradkin, M I Gusakov, Yu V Kaplin, V A Kachanov, V A Kheymits, M D Leonov, A A Longo, F Mazets, E P Maestro, P Marrocchesi, P Mereminskiy, I A Mikhailov, V V Moiseev, A A Mocchiutti, E Mori, N Moskalenko, I V P Yu Naumov Papini, P Picozza, P Rodin, V G Runtso, M F Sparvoli, R Spillantini, P Suchkov, S I Tavani, M Topchiev, N P Vacchi, A Vannuccini, E Yurkin, Yu T Zampa, N Zverev, V G Zirakashvili, V N |
| description | The GAMMA-400 gamma-ray telescope is designed to measure the fluxes of gamma rays and cosmic-ray electrons + positrons, which can be produced by annihilation or decay of the dark matter particles, as well as to survey the celestial sphere in order to study point and extended sources of gamma rays, measure energy spectra of Galactic and extragalactic diffuse gamma-ray emission, gamma-ray bursts, and gamma-ray emission from the Sun. The GAMMA-400 covers the energy range from 100 MeV to 3000 GeV. Its angular resolution is ~0.01 deg (E{\gamma} > 100 GeV), the energy resolution ~1% (E{\gamma} > 10 GeV), and the proton rejection factor ~10E6. GAMMA-400 will be installed on the Russian space platform Navigator. The beginning of observations is planned for 2018. |
| doi_str_mv | 10.48550/arxiv.1210.1457 |
| format | Article |
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The GAMMA-400 covers the energy range from 100 MeV to 3000 GeV. Its angular resolution is ~0.01 deg (E{\gamma} > 100 GeV), the energy resolution ~1% (E{\gamma} > 10 GeV), and the proton rejection factor ~10E6. GAMMA-400 will be installed on the Russian space platform Navigator. The beginning of observations is planned for 2018.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1210.1457</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Angular resolution ; Celestial sphere ; Cosmic rays ; Dark matter ; Emission ; Energy measurement ; Energy resolution ; Energy spectra ; Fluxes ; Gamma ray bursts ; Gamma ray telescopes ; Gamma rays ; Particle decay ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Positrons ; Space stations ; Space telescopes</subject><ispartof>arXiv.org, 2012-10</ispartof><rights>2012. 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Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,778,782,883,27908</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.1210.1457$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1063/1.4792586$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Galper, A M</creatorcontrib><creatorcontrib>Adriani, O</creatorcontrib><creatorcontrib>Aptekar, R L</creatorcontrib><creatorcontrib>Arkhangelskaja, I V</creatorcontrib><creatorcontrib>Arkhangelskiy, A I</creatorcontrib><creatorcontrib>Boezio, M</creatorcontrib><creatorcontrib>Bonvicini, V</creatorcontrib><creatorcontrib>Boyarchuk, K A</creatorcontrib><creatorcontrib>Fradkin, M I</creatorcontrib><creatorcontrib>Gusakov, Yu V</creatorcontrib><creatorcontrib>Kaplin, V A</creatorcontrib><creatorcontrib>Kachanov, V A</creatorcontrib><creatorcontrib>Kheymits, M D</creatorcontrib><creatorcontrib>Leonov, A A</creatorcontrib><creatorcontrib>Longo, F</creatorcontrib><creatorcontrib>Mazets, E P</creatorcontrib><creatorcontrib>Maestro, P</creatorcontrib><creatorcontrib>Marrocchesi, P</creatorcontrib><creatorcontrib>Mereminskiy, I A</creatorcontrib><creatorcontrib>Mikhailov, V V</creatorcontrib><creatorcontrib>Moiseev, A A</creatorcontrib><creatorcontrib>Mocchiutti, E</creatorcontrib><creatorcontrib>Mori, N</creatorcontrib><creatorcontrib>Moskalenko, I V</creatorcontrib><creatorcontrib>P Yu Naumov</creatorcontrib><creatorcontrib>Papini, P</creatorcontrib><creatorcontrib>Picozza, P</creatorcontrib><creatorcontrib>Rodin, V G</creatorcontrib><creatorcontrib>Runtso, M F</creatorcontrib><creatorcontrib>Sparvoli, R</creatorcontrib><creatorcontrib>Spillantini, P</creatorcontrib><creatorcontrib>Suchkov, S I</creatorcontrib><creatorcontrib>Tavani, M</creatorcontrib><creatorcontrib>Topchiev, N P</creatorcontrib><creatorcontrib>Vacchi, A</creatorcontrib><creatorcontrib>Vannuccini, E</creatorcontrib><creatorcontrib>Yurkin, Yu T</creatorcontrib><creatorcontrib>Zampa, N</creatorcontrib><creatorcontrib>Zverev, V G</creatorcontrib><creatorcontrib>Zirakashvili, V N</creatorcontrib><title>Design and Performance of the GAMMA-400 Gamma-Ray Telescope for the Dark Matter Searches</title><title>arXiv.org</title><description>The GAMMA-400 gamma-ray telescope is designed to measure the fluxes of gamma rays and cosmic-ray electrons + positrons, which can be produced by annihilation or decay of the dark matter particles, as well as to survey the celestial sphere in order to study point and extended sources of gamma rays, measure energy spectra of Galactic and extragalactic diffuse gamma-ray emission, gamma-ray bursts, and gamma-ray emission from the Sun. 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The beginning of observations is planned for 2018.</description><subject>Angular resolution</subject><subject>Celestial sphere</subject><subject>Cosmic rays</subject><subject>Dark matter</subject><subject>Emission</subject><subject>Energy measurement</subject><subject>Energy resolution</subject><subject>Energy spectra</subject><subject>Fluxes</subject><subject>Gamma ray bursts</subject><subject>Gamma ray telescopes</subject><subject>Gamma rays</subject><subject>Particle decay</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Positrons</subject><subject>Space stations</subject><subject>Space telescopes</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotj0FPwkAQhTcmJhLk7sls4rk4nd0tu0cCiiYQjXLw1kzbWQFpi9ti5N9bwNNLXr68vE-ImxiG2hoD9xR-1z_DGLsi1mZ0IXqoVBxZjXglBk2zAQBMRmiM6omPKTfrz0pSVchXDr4OJVU5y9rLdsVyNl4sxpEGkDMqS4re6CCXvOUmr3csO_pETSl8yQW1LQf5zhTyFTfX4tLTtuHBf_bF8vFhOXmK5i-z58l4HpGJMSpQJ6awmbaZR--MQk_O5l7ZnMkjMGZAxmnjHcWFc5ZAgU5sZr1nB6j64vY8e7JOd2FdUjikR_v0aN8Bd2dgF-rvPTdtuqn3oeoupQgWExyBQvUHBiFawA</recordid><startdate>20121010</startdate><enddate>20121010</enddate><creator>Galper, A M</creator><creator>Adriani, O</creator><creator>Aptekar, R L</creator><creator>Arkhangelskaja, I V</creator><creator>Arkhangelskiy, A I</creator><creator>Boezio, M</creator><creator>Bonvicini, V</creator><creator>Boyarchuk, K A</creator><creator>Fradkin, M I</creator><creator>Gusakov, Yu V</creator><creator>Kaplin, V A</creator><creator>Kachanov, V A</creator><creator>Kheymits, M D</creator><creator>Leonov, A A</creator><creator>Longo, F</creator><creator>Mazets, E P</creator><creator>Maestro, P</creator><creator>Marrocchesi, P</creator><creator>Mereminskiy, I A</creator><creator>Mikhailov, V V</creator><creator>Moiseev, A A</creator><creator>Mocchiutti, E</creator><creator>Mori, N</creator><creator>Moskalenko, I V</creator><creator>P Yu Naumov</creator><creator>Papini, P</creator><creator>Picozza, P</creator><creator>Rodin, V G</creator><creator>Runtso, M F</creator><creator>Sparvoli, R</creator><creator>Spillantini, P</creator><creator>Suchkov, S I</creator><creator>Tavani, M</creator><creator>Topchiev, N P</creator><creator>Vacchi, A</creator><creator>Vannuccini, E</creator><creator>Yurkin, Yu T</creator><creator>Zampa, N</creator><creator>Zverev, V G</creator><creator>Zirakashvili, V N</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20121010</creationdate><title>Design and Performance of the GAMMA-400 Gamma-Ray Telescope for the Dark Matter Searches</title><author>Galper, A M ; Adriani, O ; Aptekar, R L ; Arkhangelskaja, I V ; Arkhangelskiy, A I ; Boezio, M ; Bonvicini, V ; Boyarchuk, K A ; Fradkin, M I ; Gusakov, Yu V ; Kaplin, V A ; Kachanov, V A ; Kheymits, M D ; Leonov, A A ; Longo, F ; Mazets, E P ; Maestro, P ; Marrocchesi, P ; Mereminskiy, I A ; Mikhailov, V V ; Moiseev, A A ; Mocchiutti, E ; Mori, N ; Moskalenko, I V ; P Yu Naumov ; Papini, P ; Picozza, P ; Rodin, V G ; Runtso, M F ; Sparvoli, R ; Spillantini, P ; Suchkov, S I ; Tavani, M ; Topchiev, N P ; Vacchi, A ; Vannuccini, E ; Yurkin, Yu T ; Zampa, N ; Zverev, V G ; Zirakashvili, V N</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a512-d2465d8b48bf2f9532fa98cf38ceaf20e2b0a5945f9a1d998a030468b8ffe9023</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Angular resolution</topic><topic>Celestial sphere</topic><topic>Cosmic rays</topic><topic>Dark matter</topic><topic>Emission</topic><topic>Energy measurement</topic><topic>Energy resolution</topic><topic>Energy spectra</topic><topic>Fluxes</topic><topic>Gamma ray bursts</topic><topic>Gamma ray telescopes</topic><topic>Gamma rays</topic><topic>Particle decay</topic><topic>Physics - 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| recordid | cdi_arxiv_primary_1210_1457 |
| source | arXiv.org; Free E- Journals |
| subjects | Angular resolution Celestial sphere Cosmic rays Dark matter Emission Energy measurement Energy resolution Energy spectra Fluxes Gamma ray bursts Gamma ray telescopes Gamma rays Particle decay Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Positrons Space stations Space telescopes |
| title | Design and Performance of the GAMMA-400 Gamma-Ray Telescope for the Dark Matter Searches |
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