The GAMMA-400 experiment: Status and prospects
Abstract The development of the GAMMA-400 γ-ray telescope continues. The GAMMA-400 is designed to measure fluxes of γ-rays and the electron-positron cosmic-ray component possibly associated with annihilation or decay of dark matter particles; and to search for and study in detail discrete γ-ray sour...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Topchiev, N. P. [verfasserIn] Galper, A. M. [verfasserIn] Bonvicini, V. [verfasserIn] Adriani, O. [verfasserIn] Aptekar, R. L. [verfasserIn] Arkhangelskaja, I. V. [verfasserIn] Arkhangelskiy, A. I. [verfasserIn] Bergstrom, L. [verfasserIn] Berti, E. [verfasserIn] Bigongiari, G. [verfasserIn] Bobkov, S. G. [verfasserIn] Bogomolov, E. A. [verfasserIn] Boezio, M. [verfasserIn] Bongi, M. [verfasserIn] Bonechi, S. [verfasserIn] Bottai, S. [verfasserIn] Boyarchuk, K. A. [verfasserIn] Vacchi, A. [verfasserIn] Vannuccini, E. [verfasserIn] Vasilyev, G. I. [verfasserIn] Castellini, G. [verfasserIn] Cattaneo, P. W. [verfasserIn] Cumani, P. [verfasserIn] Dedenko, G. L. [verfasserIn] Dogiel, V. A. [verfasserIn] De Donato, C. [verfasserIn] Hnatyk, B. I. [verfasserIn] Gorbunov, M. S. [verfasserIn] Gusakov, Yu. V. [verfasserIn] Zampa, N. [verfasserIn] Zverev, V. G. [verfasserIn] Zirakashvili, V. N. [verfasserIn] Kadilin, V. V. [verfasserIn] Kaplin, V. A. [verfasserIn] Kaplun, A. A. [verfasserIn] Korepanov, V. E. [verfasserIn] Larsson, J. [verfasserIn] Leonov, A. A. [verfasserIn] Loginov, V. A. [verfasserIn] Longo, F. [verfasserIn] Maestro, P. [verfasserIn] Marrocchesi, P. S. [verfasserIn] Mikhailov, V. V. [verfasserIn] Mocchiutti, E. [verfasserIn] Moiseev, A. A. [verfasserIn] Mori, N. [verfasserIn] Moskalenko, I. V. [verfasserIn] Naumov, P. Yu. [verfasserIn] Papini, P. [verfasserIn] Picozza, P. [verfasserIn] Pearce, M. [verfasserIn] Popov, A. V. [verfasserIn] Ryde, F. [verfasserIn] Rappoldi, A. [verfasserIn] Ricciarini, S. [verfasserIn] Runtso, M. F. [verfasserIn] Serdin, O. V. [verfasserIn] Sparvoli, R. [verfasserIn] Spillantini, P. [verfasserIn] Suchkov, S. I. [verfasserIn] Tavani, M. [verfasserIn] Taraskin, A. A. [verfasserIn] Tiberio, A. [verfasserIn] Tyurin, E. M. [verfasserIn] Ulanov, M. V. [verfasserIn] Fuglesang, Ch. [verfasserIn] Kheymits, M. D. [verfasserIn] Yurkin, Yu. T. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Bulletin of the Russian Academy of Sciences - New York, NY : Allerton Press, 2007, 79(2015), 3 vom: März, Seite 417-420 |
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| Übergeordnetes Werk: |
volume:79 ; year:2015 ; number:3 ; month:03 ; pages:417-420 |
| Links: |
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| DOI / URN: |
10.3103/S1062873815030429 |
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| Katalog-ID: |
SPR023173734 |
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| 100 | 1 | |a Topchiev, N. P. |e verfasserin |4 aut | |
| 245 | 1 | 4 | |a The GAMMA-400 experiment: Status and prospects |
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| 520 | |a Abstract The development of the GAMMA-400 γ-ray telescope continues. The GAMMA-400 is designed to measure fluxes of γ-rays and the electron-positron cosmic-ray component possibly associated with annihilation or decay of dark matter particles; and to search for and study in detail discrete γ-ray sources, to measure the energy spectra of Galactic and extragalactic diffuse γ-rays, and to study γ-ray bursts and γ-rays from the active Sun. The energy range for measuring γ-rays and electrons (positrons) is from 100 MeV to 3000 GeV. For 100-GeV γ-rays, the γ-ray telescope has an angular resolution of ∼0.01°, an energy resolution of ∼1%, and a proton rejection factor of ∼5 × $ 10^{5} $. The GAMMA-400 will be installed onboard the Russian Space Observatory. | ||
| 650 | 4 | |a Galactic Center |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Neutron Detector |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Dark Matter Particle |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Scientific Complex |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Strip Pitch |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Galper, A. M. |e verfasserin |4 aut | |
| 700 | 1 | |a Bonvicini, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Adriani, O. |e verfasserin |4 aut | |
| 700 | 1 | |a Aptekar, R. L. |e verfasserin |4 aut | |
| 700 | 1 | |a Arkhangelskaja, I. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Arkhangelskiy, A. I. |e verfasserin |4 aut | |
| 700 | 1 | |a Bergstrom, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Berti, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Bigongiari, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Bobkov, S. G. |e verfasserin |4 aut | |
| 700 | 1 | |a Bogomolov, E. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Boezio, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Bongi, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Bonechi, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Bottai, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Boyarchuk, K. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Vacchi, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Vannuccini, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Vasilyev, G. I. |e verfasserin |4 aut | |
| 700 | 1 | |a Castellini, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Cattaneo, P. W. |e verfasserin |4 aut | |
| 700 | 1 | |a Cumani, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Dedenko, G. L. |e verfasserin |4 aut | |
| 700 | 1 | |a Dogiel, V. A. |e verfasserin |4 aut | |
| 700 | 1 | |a De Donato, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Hnatyk, B. I. |e verfasserin |4 aut | |
| 700 | 1 | |a Gorbunov, M. S. |e verfasserin |4 aut | |
| 700 | 1 | |a Gusakov, Yu. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Zampa, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Zverev, V. G. |e verfasserin |4 aut | |
| 700 | 1 | |a Zirakashvili, V. N. |e verfasserin |4 aut | |
| 700 | 1 | |a Kadilin, V. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Kaplin, V. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Kaplun, A. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Korepanov, V. E. |e verfasserin |4 aut | |
| 700 | 1 | |a Larsson, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Leonov, A. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Loginov, V. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Longo, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Maestro, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Marrocchesi, P. S. |e verfasserin |4 aut | |
| 700 | 1 | |a Mikhailov, V. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Mocchiutti, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Moiseev, A. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Mori, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Moskalenko, I. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Naumov, P. Yu. |e verfasserin |4 aut | |
| 700 | 1 | |a Papini, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Picozza, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Pearce, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Popov, A. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Ryde, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Rappoldi, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Ricciarini, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Runtso, M. F. |e verfasserin |4 aut | |
| 700 | 1 | |a Serdin, O. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Sparvoli, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Spillantini, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Suchkov, S. I. |e verfasserin |4 aut | |
| 700 | 1 | |a Tavani, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Taraskin, A. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Tiberio, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Tyurin, E. M. |e verfasserin |4 aut | |
| 700 | 1 | |a Ulanov, M. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Fuglesang, Ch. |e verfasserin |4 aut | |
| 700 | 1 | |a Kheymits, M. D. |e verfasserin |4 aut | |
| 700 | 1 | |a Yurkin, Yu. T. |e verfasserin |4 aut | |
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10.3103/S1062873815030429 doi (DE-627)SPR023173734 (SPR)S1062873815030429-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Topchiev, N. P. verfasserin aut The GAMMA-400 experiment: Status and prospects 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The development of the GAMMA-400 γ-ray telescope continues. The GAMMA-400 is designed to measure fluxes of γ-rays and the electron-positron cosmic-ray component possibly associated with annihilation or decay of dark matter particles; and to search for and study in detail discrete γ-ray sources, to measure the energy spectra of Galactic and extragalactic diffuse γ-rays, and to study γ-ray bursts and γ-rays from the active Sun. The energy range for measuring γ-rays and electrons (positrons) is from 100 MeV to 3000 GeV. For 100-GeV γ-rays, the γ-ray telescope has an angular resolution of ∼0.01°, an energy resolution of ∼1%, and a proton rejection factor of ∼5 × $ 10^{5} $. The GAMMA-400 will be installed onboard the Russian Space Observatory. Galactic Center (dpeaa)DE-He213 Neutron Detector (dpeaa)DE-He213 Dark Matter Particle (dpeaa)DE-He213 Scientific Complex (dpeaa)DE-He213 Strip Pitch (dpeaa)DE-He213 Galper, A. M. verfasserin aut Bonvicini, V. verfasserin aut Adriani, O. verfasserin aut Aptekar, R. L. verfasserin aut Arkhangelskaja, I. V. verfasserin aut Arkhangelskiy, A. I. verfasserin aut Bergstrom, L. verfasserin aut Berti, E. verfasserin aut Bigongiari, G. verfasserin aut Bobkov, S. G. verfasserin aut Bogomolov, E. A. verfasserin aut Boezio, M. verfasserin aut Bongi, M. verfasserin aut Bonechi, S. verfasserin aut Bottai, S. verfasserin aut Boyarchuk, K. A. verfasserin aut Vacchi, A. verfasserin aut Vannuccini, E. verfasserin aut Vasilyev, G. I. verfasserin aut Castellini, G. verfasserin aut Cattaneo, P. W. verfasserin aut Cumani, P. verfasserin aut Dedenko, G. L. verfasserin aut Dogiel, V. A. verfasserin aut De Donato, C. verfasserin aut Hnatyk, B. I. verfasserin aut Gorbunov, M. S. verfasserin aut Gusakov, Yu. V. verfasserin aut Zampa, N. verfasserin aut Zverev, V. G. verfasserin aut Zirakashvili, V. N. verfasserin aut Kadilin, V. V. verfasserin aut Kaplin, V. A. verfasserin aut Kaplun, A. A. verfasserin aut Korepanov, V. E. verfasserin aut Larsson, J. verfasserin aut Leonov, A. A. verfasserin aut Loginov, V. A. verfasserin aut Longo, F. verfasserin aut Maestro, P. verfasserin aut Marrocchesi, P. S. verfasserin aut Mikhailov, V. V. verfasserin aut Mocchiutti, E. verfasserin aut Moiseev, A. A. verfasserin aut Mori, N. verfasserin aut Moskalenko, I. V. verfasserin aut Naumov, P. Yu. verfasserin aut Papini, P. verfasserin aut Picozza, P. verfasserin aut Pearce, M. verfasserin aut Popov, A. V. verfasserin aut Ryde, F. verfasserin aut Rappoldi, A. verfasserin aut Ricciarini, S. verfasserin aut Runtso, M. F. verfasserin aut Serdin, O. V. verfasserin aut Sparvoli, R. verfasserin aut Spillantini, P. verfasserin aut Suchkov, S. I. verfasserin aut Tavani, M. verfasserin aut Taraskin, A. A. verfasserin aut Tiberio, A. verfasserin aut Tyurin, E. M. verfasserin aut Ulanov, M. V. verfasserin aut Fuglesang, Ch. verfasserin aut Kheymits, M. D. verfasserin aut Yurkin, Yu. T. verfasserin aut Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 79(2015), 3 vom: März, Seite 417-420 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:79 year:2015 number:3 month:03 pages:417-420 https://dx.doi.org/10.3103/S1062873815030429 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 79 2015 3 03 417-420 |
| spelling |
10.3103/S1062873815030429 doi (DE-627)SPR023173734 (SPR)S1062873815030429-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Topchiev, N. P. verfasserin aut The GAMMA-400 experiment: Status and prospects 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The development of the GAMMA-400 γ-ray telescope continues. The GAMMA-400 is designed to measure fluxes of γ-rays and the electron-positron cosmic-ray component possibly associated with annihilation or decay of dark matter particles; and to search for and study in detail discrete γ-ray sources, to measure the energy spectra of Galactic and extragalactic diffuse γ-rays, and to study γ-ray bursts and γ-rays from the active Sun. The energy range for measuring γ-rays and electrons (positrons) is from 100 MeV to 3000 GeV. For 100-GeV γ-rays, the γ-ray telescope has an angular resolution of ∼0.01°, an energy resolution of ∼1%, and a proton rejection factor of ∼5 × $ 10^{5} $. The GAMMA-400 will be installed onboard the Russian Space Observatory. Galactic Center (dpeaa)DE-He213 Neutron Detector (dpeaa)DE-He213 Dark Matter Particle (dpeaa)DE-He213 Scientific Complex (dpeaa)DE-He213 Strip Pitch (dpeaa)DE-He213 Galper, A. M. verfasserin aut Bonvicini, V. verfasserin aut Adriani, O. verfasserin aut Aptekar, R. L. verfasserin aut Arkhangelskaja, I. V. verfasserin aut Arkhangelskiy, A. I. verfasserin aut Bergstrom, L. verfasserin aut Berti, E. verfasserin aut Bigongiari, G. verfasserin aut Bobkov, S. G. verfasserin aut Bogomolov, E. A. verfasserin aut Boezio, M. verfasserin aut Bongi, M. verfasserin aut Bonechi, S. verfasserin aut Bottai, S. verfasserin aut Boyarchuk, K. A. verfasserin aut Vacchi, A. verfasserin aut Vannuccini, E. verfasserin aut Vasilyev, G. I. verfasserin aut Castellini, G. verfasserin aut Cattaneo, P. W. verfasserin aut Cumani, P. verfasserin aut Dedenko, G. L. verfasserin aut Dogiel, V. A. verfasserin aut De Donato, C. verfasserin aut Hnatyk, B. I. verfasserin aut Gorbunov, M. S. verfasserin aut Gusakov, Yu. V. verfasserin aut Zampa, N. verfasserin aut Zverev, V. G. verfasserin aut Zirakashvili, V. N. verfasserin aut Kadilin, V. V. verfasserin aut Kaplin, V. A. verfasserin aut Kaplun, A. A. verfasserin aut Korepanov, V. E. verfasserin aut Larsson, J. verfasserin aut Leonov, A. A. verfasserin aut Loginov, V. A. verfasserin aut Longo, F. verfasserin aut Maestro, P. verfasserin aut Marrocchesi, P. S. verfasserin aut Mikhailov, V. V. verfasserin aut Mocchiutti, E. verfasserin aut Moiseev, A. A. verfasserin aut Mori, N. verfasserin aut Moskalenko, I. V. verfasserin aut Naumov, P. Yu. verfasserin aut Papini, P. verfasserin aut Picozza, P. verfasserin aut Pearce, M. verfasserin aut Popov, A. V. verfasserin aut Ryde, F. verfasserin aut Rappoldi, A. verfasserin aut Ricciarini, S. verfasserin aut Runtso, M. F. verfasserin aut Serdin, O. V. verfasserin aut Sparvoli, R. verfasserin aut Spillantini, P. verfasserin aut Suchkov, S. I. verfasserin aut Tavani, M. verfasserin aut Taraskin, A. A. verfasserin aut Tiberio, A. verfasserin aut Tyurin, E. M. verfasserin aut Ulanov, M. V. verfasserin aut Fuglesang, Ch. verfasserin aut Kheymits, M. D. verfasserin aut Yurkin, Yu. T. verfasserin aut Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 79(2015), 3 vom: März, Seite 417-420 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:79 year:2015 number:3 month:03 pages:417-420 https://dx.doi.org/10.3103/S1062873815030429 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 79 2015 3 03 417-420 |
| allfields_unstemmed |
10.3103/S1062873815030429 doi (DE-627)SPR023173734 (SPR)S1062873815030429-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Topchiev, N. P. verfasserin aut The GAMMA-400 experiment: Status and prospects 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The development of the GAMMA-400 γ-ray telescope continues. The GAMMA-400 is designed to measure fluxes of γ-rays and the electron-positron cosmic-ray component possibly associated with annihilation or decay of dark matter particles; and to search for and study in detail discrete γ-ray sources, to measure the energy spectra of Galactic and extragalactic diffuse γ-rays, and to study γ-ray bursts and γ-rays from the active Sun. The energy range for measuring γ-rays and electrons (positrons) is from 100 MeV to 3000 GeV. For 100-GeV γ-rays, the γ-ray telescope has an angular resolution of ∼0.01°, an energy resolution of ∼1%, and a proton rejection factor of ∼5 × $ 10^{5} $. The GAMMA-400 will be installed onboard the Russian Space Observatory. Galactic Center (dpeaa)DE-He213 Neutron Detector (dpeaa)DE-He213 Dark Matter Particle (dpeaa)DE-He213 Scientific Complex (dpeaa)DE-He213 Strip Pitch (dpeaa)DE-He213 Galper, A. M. verfasserin aut Bonvicini, V. verfasserin aut Adriani, O. verfasserin aut Aptekar, R. L. verfasserin aut Arkhangelskaja, I. V. verfasserin aut Arkhangelskiy, A. I. verfasserin aut Bergstrom, L. verfasserin aut Berti, E. verfasserin aut Bigongiari, G. verfasserin aut Bobkov, S. G. verfasserin aut Bogomolov, E. A. verfasserin aut Boezio, M. verfasserin aut Bongi, M. verfasserin aut Bonechi, S. verfasserin aut Bottai, S. verfasserin aut Boyarchuk, K. A. verfasserin aut Vacchi, A. verfasserin aut Vannuccini, E. verfasserin aut Vasilyev, G. I. verfasserin aut Castellini, G. verfasserin aut Cattaneo, P. W. verfasserin aut Cumani, P. verfasserin aut Dedenko, G. L. verfasserin aut Dogiel, V. A. verfasserin aut De Donato, C. verfasserin aut Hnatyk, B. I. verfasserin aut Gorbunov, M. S. verfasserin aut Gusakov, Yu. V. verfasserin aut Zampa, N. verfasserin aut Zverev, V. G. verfasserin aut Zirakashvili, V. N. verfasserin aut Kadilin, V. V. verfasserin aut Kaplin, V. A. verfasserin aut Kaplun, A. A. verfasserin aut Korepanov, V. E. verfasserin aut Larsson, J. verfasserin aut Leonov, A. A. verfasserin aut Loginov, V. A. verfasserin aut Longo, F. verfasserin aut Maestro, P. verfasserin aut Marrocchesi, P. S. verfasserin aut Mikhailov, V. V. verfasserin aut Mocchiutti, E. verfasserin aut Moiseev, A. A. verfasserin aut Mori, N. verfasserin aut Moskalenko, I. V. verfasserin aut Naumov, P. Yu. verfasserin aut Papini, P. verfasserin aut Picozza, P. verfasserin aut Pearce, M. verfasserin aut Popov, A. V. verfasserin aut Ryde, F. verfasserin aut Rappoldi, A. verfasserin aut Ricciarini, S. verfasserin aut Runtso, M. F. verfasserin aut Serdin, O. V. verfasserin aut Sparvoli, R. verfasserin aut Spillantini, P. verfasserin aut Suchkov, S. I. verfasserin aut Tavani, M. verfasserin aut Taraskin, A. A. verfasserin aut Tiberio, A. verfasserin aut Tyurin, E. M. verfasserin aut Ulanov, M. V. verfasserin aut Fuglesang, Ch. verfasserin aut Kheymits, M. D. verfasserin aut Yurkin, Yu. T. verfasserin aut Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 79(2015), 3 vom: März, Seite 417-420 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:79 year:2015 number:3 month:03 pages:417-420 https://dx.doi.org/10.3103/S1062873815030429 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 79 2015 3 03 417-420 |
| allfieldsGer |
10.3103/S1062873815030429 doi (DE-627)SPR023173734 (SPR)S1062873815030429-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Topchiev, N. P. verfasserin aut The GAMMA-400 experiment: Status and prospects 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The development of the GAMMA-400 γ-ray telescope continues. The GAMMA-400 is designed to measure fluxes of γ-rays and the electron-positron cosmic-ray component possibly associated with annihilation or decay of dark matter particles; and to search for and study in detail discrete γ-ray sources, to measure the energy spectra of Galactic and extragalactic diffuse γ-rays, and to study γ-ray bursts and γ-rays from the active Sun. The energy range for measuring γ-rays and electrons (positrons) is from 100 MeV to 3000 GeV. For 100-GeV γ-rays, the γ-ray telescope has an angular resolution of ∼0.01°, an energy resolution of ∼1%, and a proton rejection factor of ∼5 × $ 10^{5} $. The GAMMA-400 will be installed onboard the Russian Space Observatory. Galactic Center (dpeaa)DE-He213 Neutron Detector (dpeaa)DE-He213 Dark Matter Particle (dpeaa)DE-He213 Scientific Complex (dpeaa)DE-He213 Strip Pitch (dpeaa)DE-He213 Galper, A. M. verfasserin aut Bonvicini, V. verfasserin aut Adriani, O. verfasserin aut Aptekar, R. L. verfasserin aut Arkhangelskaja, I. V. verfasserin aut Arkhangelskiy, A. I. verfasserin aut Bergstrom, L. verfasserin aut Berti, E. verfasserin aut Bigongiari, G. verfasserin aut Bobkov, S. G. verfasserin aut Bogomolov, E. A. verfasserin aut Boezio, M. verfasserin aut Bongi, M. verfasserin aut Bonechi, S. verfasserin aut Bottai, S. verfasserin aut Boyarchuk, K. A. verfasserin aut Vacchi, A. verfasserin aut Vannuccini, E. verfasserin aut Vasilyev, G. I. verfasserin aut Castellini, G. verfasserin aut Cattaneo, P. W. verfasserin aut Cumani, P. verfasserin aut Dedenko, G. L. verfasserin aut Dogiel, V. A. verfasserin aut De Donato, C. verfasserin aut Hnatyk, B. I. verfasserin aut Gorbunov, M. S. verfasserin aut Gusakov, Yu. V. verfasserin aut Zampa, N. verfasserin aut Zverev, V. G. verfasserin aut Zirakashvili, V. N. verfasserin aut Kadilin, V. V. verfasserin aut Kaplin, V. A. verfasserin aut Kaplun, A. A. verfasserin aut Korepanov, V. E. verfasserin aut Larsson, J. verfasserin aut Leonov, A. A. verfasserin aut Loginov, V. A. verfasserin aut Longo, F. verfasserin aut Maestro, P. verfasserin aut Marrocchesi, P. S. verfasserin aut Mikhailov, V. V. verfasserin aut Mocchiutti, E. verfasserin aut Moiseev, A. A. verfasserin aut Mori, N. verfasserin aut Moskalenko, I. V. verfasserin aut Naumov, P. Yu. verfasserin aut Papini, P. verfasserin aut Picozza, P. verfasserin aut Pearce, M. verfasserin aut Popov, A. V. verfasserin aut Ryde, F. verfasserin aut Rappoldi, A. verfasserin aut Ricciarini, S. verfasserin aut Runtso, M. F. verfasserin aut Serdin, O. V. verfasserin aut Sparvoli, R. verfasserin aut Spillantini, P. verfasserin aut Suchkov, S. I. verfasserin aut Tavani, M. verfasserin aut Taraskin, A. A. verfasserin aut Tiberio, A. verfasserin aut Tyurin, E. M. verfasserin aut Ulanov, M. V. verfasserin aut Fuglesang, Ch. verfasserin aut Kheymits, M. D. verfasserin aut Yurkin, Yu. T. verfasserin aut Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 79(2015), 3 vom: März, Seite 417-420 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:79 year:2015 number:3 month:03 pages:417-420 https://dx.doi.org/10.3103/S1062873815030429 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 79 2015 3 03 417-420 |
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10.3103/S1062873815030429 doi (DE-627)SPR023173734 (SPR)S1062873815030429-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Topchiev, N. P. verfasserin aut The GAMMA-400 experiment: Status and prospects 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The development of the GAMMA-400 γ-ray telescope continues. The GAMMA-400 is designed to measure fluxes of γ-rays and the electron-positron cosmic-ray component possibly associated with annihilation or decay of dark matter particles; and to search for and study in detail discrete γ-ray sources, to measure the energy spectra of Galactic and extragalactic diffuse γ-rays, and to study γ-ray bursts and γ-rays from the active Sun. The energy range for measuring γ-rays and electrons (positrons) is from 100 MeV to 3000 GeV. For 100-GeV γ-rays, the γ-ray telescope has an angular resolution of ∼0.01°, an energy resolution of ∼1%, and a proton rejection factor of ∼5 × $ 10^{5} $. The GAMMA-400 will be installed onboard the Russian Space Observatory. Galactic Center (dpeaa)DE-He213 Neutron Detector (dpeaa)DE-He213 Dark Matter Particle (dpeaa)DE-He213 Scientific Complex (dpeaa)DE-He213 Strip Pitch (dpeaa)DE-He213 Galper, A. M. verfasserin aut Bonvicini, V. verfasserin aut Adriani, O. verfasserin aut Aptekar, R. L. verfasserin aut Arkhangelskaja, I. V. verfasserin aut Arkhangelskiy, A. I. verfasserin aut Bergstrom, L. verfasserin aut Berti, E. verfasserin aut Bigongiari, G. verfasserin aut Bobkov, S. G. verfasserin aut Bogomolov, E. A. verfasserin aut Boezio, M. verfasserin aut Bongi, M. verfasserin aut Bonechi, S. verfasserin aut Bottai, S. verfasserin aut Boyarchuk, K. A. verfasserin aut Vacchi, A. verfasserin aut Vannuccini, E. verfasserin aut Vasilyev, G. I. verfasserin aut Castellini, G. verfasserin aut Cattaneo, P. W. verfasserin aut Cumani, P. verfasserin aut Dedenko, G. L. verfasserin aut Dogiel, V. A. verfasserin aut De Donato, C. verfasserin aut Hnatyk, B. I. verfasserin aut Gorbunov, M. S. verfasserin aut Gusakov, Yu. V. verfasserin aut Zampa, N. verfasserin aut Zverev, V. G. verfasserin aut Zirakashvili, V. N. verfasserin aut Kadilin, V. V. verfasserin aut Kaplin, V. A. verfasserin aut Kaplun, A. A. verfasserin aut Korepanov, V. E. verfasserin aut Larsson, J. verfasserin aut Leonov, A. A. verfasserin aut Loginov, V. A. verfasserin aut Longo, F. verfasserin aut Maestro, P. verfasserin aut Marrocchesi, P. S. verfasserin aut Mikhailov, V. V. verfasserin aut Mocchiutti, E. verfasserin aut Moiseev, A. A. verfasserin aut Mori, N. verfasserin aut Moskalenko, I. V. verfasserin aut Naumov, P. Yu. verfasserin aut Papini, P. verfasserin aut Picozza, P. verfasserin aut Pearce, M. verfasserin aut Popov, A. V. verfasserin aut Ryde, F. verfasserin aut Rappoldi, A. verfasserin aut Ricciarini, S. verfasserin aut Runtso, M. F. verfasserin aut Serdin, O. V. verfasserin aut Sparvoli, R. verfasserin aut Spillantini, P. verfasserin aut Suchkov, S. I. verfasserin aut Tavani, M. verfasserin aut Taraskin, A. A. verfasserin aut Tiberio, A. verfasserin aut Tyurin, E. M. verfasserin aut Ulanov, M. V. verfasserin aut Fuglesang, Ch. verfasserin aut Kheymits, M. D. verfasserin aut Yurkin, Yu. T. verfasserin aut Enthalten in Bulletin of the Russian Academy of Sciences New York, NY : Allerton Press, 2007 79(2015), 3 vom: März, Seite 417-420 (DE-627)556723872 (DE-600)2403169-0 1934-9432 nnns volume:79 year:2015 number:3 month:03 pages:417-420 https://dx.doi.org/10.3103/S1062873815030429 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 79 2015 3 03 417-420 |
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Topchiev, N. P. @@aut@@ Galper, A. M. @@aut@@ Bonvicini, V. @@aut@@ Adriani, O. @@aut@@ Aptekar, R. L. @@aut@@ Arkhangelskaja, I. V. @@aut@@ Arkhangelskiy, A. I. @@aut@@ Bergstrom, L. @@aut@@ Berti, E. @@aut@@ Bigongiari, G. @@aut@@ Bobkov, S. G. @@aut@@ Bogomolov, E. A. @@aut@@ Boezio, M. @@aut@@ Bongi, M. @@aut@@ Bonechi, S. @@aut@@ Bottai, S. @@aut@@ Boyarchuk, K. A. @@aut@@ Vacchi, A. @@aut@@ Vannuccini, E. @@aut@@ Vasilyev, G. I. @@aut@@ Castellini, G. @@aut@@ Cattaneo, P. W. @@aut@@ Cumani, P. @@aut@@ Dedenko, G. L. @@aut@@ Dogiel, V. A. @@aut@@ De Donato, C. @@aut@@ Hnatyk, B. I. @@aut@@ Gorbunov, M. S. @@aut@@ Gusakov, Yu. V. @@aut@@ Zampa, N. @@aut@@ Zverev, V. G. @@aut@@ Zirakashvili, V. N. @@aut@@ Kadilin, V. V. @@aut@@ Kaplin, V. A. @@aut@@ Kaplun, A. A. @@aut@@ Korepanov, V. E. @@aut@@ Larsson, J. @@aut@@ Leonov, A. A. @@aut@@ Loginov, V. A. @@aut@@ Longo, F. @@aut@@ Maestro, P. @@aut@@ Marrocchesi, P. S. @@aut@@ Mikhailov, V. V. @@aut@@ Mocchiutti, E. @@aut@@ Moiseev, A. A. @@aut@@ Mori, N. @@aut@@ Moskalenko, I. V. @@aut@@ Naumov, P. Yu. @@aut@@ Papini, P. @@aut@@ Picozza, P. @@aut@@ Pearce, M. @@aut@@ Popov, A. V. @@aut@@ Ryde, F. @@aut@@ Rappoldi, A. @@aut@@ Ricciarini, S. @@aut@@ Runtso, M. F. @@aut@@ Serdin, O. V. @@aut@@ Sparvoli, R. @@aut@@ Spillantini, P. @@aut@@ Suchkov, S. I. @@aut@@ Tavani, M. @@aut@@ Taraskin, A. A. @@aut@@ Tiberio, A. @@aut@@ Tyurin, E. M. @@aut@@ Ulanov, M. V. @@aut@@ Fuglesang, Ch. @@aut@@ Kheymits, M. D. @@aut@@ Yurkin, Yu. T. @@aut@@ |
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|
| author |
Topchiev, N. P. |
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Topchiev, N. P. Galper, A. M. Bonvicini, V. Adriani, O. Aptekar, R. L. Arkhangelskaja, I. V. Arkhangelskiy, A. I. Bergstrom, L. Berti, E. Bigongiari, G. Bobkov, S. G. Bogomolov, E. A. Boezio, M. Bongi, M. Bonechi, S. Bottai, S. Boyarchuk, K. A. Vacchi, A. Vannuccini, E. Vasilyev, G. I. Castellini, G. Cattaneo, P. W. Cumani, P. Dedenko, G. L. Dogiel, V. A. De Donato, C. Hnatyk, B. I. Gorbunov, M. S. Gusakov, Yu. V. Zampa, N. Zverev, V. G. Zirakashvili, V. N. Kadilin, V. V. Kaplin, V. A. Kaplun, A. A. Korepanov, V. E. Larsson, J. Leonov, A. A. Loginov, V. A. Longo, F. Maestro, P. Marrocchesi, P. S. Mikhailov, V. V. Mocchiutti, E. Moiseev, A. A. Mori, N. Moskalenko, I. V. Naumov, P. Yu. Papini, P. Picozza, P. Pearce, M. Popov, A. V. Ryde, F. Rappoldi, A. Ricciarini, S. Runtso, M. F. Serdin, O. V. Sparvoli, R. Spillantini, P. Suchkov, S. I. Tavani, M. Taraskin, A. A. Tiberio, A. Tyurin, E. M. Ulanov, M. V. Fuglesang, Ch. Kheymits, M. D. Yurkin, Yu. T. |
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Abstract The development of the GAMMA-400 γ-ray telescope continues. The GAMMA-400 is designed to measure fluxes of γ-rays and the electron-positron cosmic-ray component possibly associated with annihilation or decay of dark matter particles; and to search for and study in detail discrete γ-ray sources, to measure the energy spectra of Galactic and extragalactic diffuse γ-rays, and to study γ-ray bursts and γ-rays from the active Sun. The energy range for measuring γ-rays and electrons (positrons) is from 100 MeV to 3000 GeV. For 100-GeV γ-rays, the γ-ray telescope has an angular resolution of ∼0.01°, an energy resolution of ∼1%, and a proton rejection factor of ∼5 × $ 10^{5} $. The GAMMA-400 will be installed onboard the Russian Space Observatory. |
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Abstract The development of the GAMMA-400 γ-ray telescope continues. The GAMMA-400 is designed to measure fluxes of γ-rays and the electron-positron cosmic-ray component possibly associated with annihilation or decay of dark matter particles; and to search for and study in detail discrete γ-ray sources, to measure the energy spectra of Galactic and extragalactic diffuse γ-rays, and to study γ-ray bursts and γ-rays from the active Sun. The energy range for measuring γ-rays and electrons (positrons) is from 100 MeV to 3000 GeV. For 100-GeV γ-rays, the γ-ray telescope has an angular resolution of ∼0.01°, an energy resolution of ∼1%, and a proton rejection factor of ∼5 × $ 10^{5} $. The GAMMA-400 will be installed onboard the Russian Space Observatory. |
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Abstract The development of the GAMMA-400 γ-ray telescope continues. The GAMMA-400 is designed to measure fluxes of γ-rays and the electron-positron cosmic-ray component possibly associated with annihilation or decay of dark matter particles; and to search for and study in detail discrete γ-ray sources, to measure the energy spectra of Galactic and extragalactic diffuse γ-rays, and to study γ-ray bursts and γ-rays from the active Sun. The energy range for measuring γ-rays and electrons (positrons) is from 100 MeV to 3000 GeV. For 100-GeV γ-rays, the γ-ray telescope has an angular resolution of ∼0.01°, an energy resolution of ∼1%, and a proton rejection factor of ∼5 × $ 10^{5} $. The GAMMA-400 will be installed onboard the Russian Space Observatory. |
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Galper, A. M. Bonvicini, V. Adriani, O. Aptekar, R. L. Arkhangelskaja, I. V. Arkhangelskiy, A. I. Bergstrom, L. Berti, E. Bigongiari, G. Bobkov, S. G. Bogomolov, E. A. Boezio, M. Bongi, M. Bonechi, S. Bottai, S. Boyarchuk, K. A. Vacchi, A. Vannuccini, E. Vasilyev, G. I. Castellini, G. Cattaneo, P. W. Cumani, P. Dedenko, G. L. Dogiel, V. A. De Donato, C. Hnatyk, B. I. Gorbunov, M. S. Gusakov, Yu. V. Zampa, N. Zverev, V. G. Zirakashvili, V. N. Kadilin, V. V. Kaplin, V. A. Kaplun, A. A. Korepanov, V. E. Larsson, J. Leonov, A. A. Loginov, V. A. Longo, F. Maestro, P. Marrocchesi, P. S. Mikhailov, V. V. Mocchiutti, E. Moiseev, A. A. Mori, N. Moskalenko, I. V. Naumov, P. Yu Papini, P. Picozza, P. Pearce, M. Popov, A. V. Ryde, F. Rappoldi, A. Ricciarini, S. Runtso, M. F. Serdin, O. V. Sparvoli, R. Spillantini, P. Suchkov, S. I. Tavani, M. Taraskin, A. A. Tiberio, A. Tyurin, E. M. Ulanov, M. V. Fuglesang, Ch Kheymits, M. D. Yurkin, Yu. T. |
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