Precision Measurements of High-Energy Cosmic Gamma-Ray Emission with the GAMMA-400 Gamma-Ray Telescope
Abstract The GAMMA-400 γ-ray telescope installed at the Russian space observatory is intended for precision measurements in the energy range of 20 MeV–1000 GeV of γ-ray emission (with the angular and energy resolutions several times better than that of current γ-ray telescopes) from discrete sources...
Ausführliche Beschreibung
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| Autor*in: |
Galper, A. M. [verfasserIn] |
|---|
| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2017 |
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| Anmerkung: |
© Pleiades Publishing, Ltd. 2017 |
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| Übergeordnetes Werk: |
Enthalten in: Physics of atomic nuclei - Pleiades Publishing, 1993, 80(2017), 6 vom: Nov., Seite 1141-1145 |
|---|---|
| Übergeordnetes Werk: |
volume:80 ; year:2017 ; number:6 ; month:11 ; pages:1141-1145 |
| Links: |
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| DOI / URN: |
10.1134/S1063778817060096 |
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OLC2049928041 |
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| 520 | |a Abstract The GAMMA-400 γ-ray telescope installed at the Russian space observatory is intended for precision measurements in the energy range of 20 MeV–1000 GeV of γ-ray emission (with the angular and energy resolutions several times better than that of current γ-ray telescopes) from discrete sources; measurement of the energy spectra of Galactic and extragalactic diffuse γ-ray emission; studies of γ-ray emission from the active Sun; and measurements of fluxes of γ-ray emission and electron–positron cosmicray component, which are probably associated with the annihilation or decay of dark-matter particles. | ||
| 700 | 1 | |a Suchkov, S. I. |4 aut | |
| 700 | 1 | |a Topchiev, N. P. |4 aut | |
| 700 | 1 | |a Arkhangelskaja, I. V. |4 aut | |
| 700 | 1 | |a Arkhangelskiy, A. I. |4 aut | |
| 700 | 1 | |a Bakaldin, A. V. |4 aut | |
| 700 | 1 | |a Gusakov, Yu. V. |4 aut | |
| 700 | 1 | |a Dalkarov, O. D. |4 aut | |
| 700 | 1 | |a Egorov, A. E. |4 aut | |
| 700 | 1 | |a Zverev, V. G. |4 aut | |
| 700 | 1 | |a Kadilin, V. V. |4 aut | |
| 700 | 1 | |a Leonov, A. A. |4 aut | |
| 700 | 1 | |a Naumov, P. Yu. |4 aut | |
| 700 | 1 | |a Runtso, M. F. |4 aut | |
| 700 | 1 | |a Kheymits, M. D. |4 aut | |
| 700 | 1 | |a Yurkin, Yu. T. |4 aut | |
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10.1134/S1063778817060096 doi (DE-627)OLC2049928041 (DE-He213)S1063778817060096-p DE-627 ger DE-627 rakwb eng 530 VZ Galper, A. M. verfasserin aut Precision Measurements of High-Energy Cosmic Gamma-Ray Emission with the GAMMA-400 Gamma-Ray Telescope 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2017 Abstract The GAMMA-400 γ-ray telescope installed at the Russian space observatory is intended for precision measurements in the energy range of 20 MeV–1000 GeV of γ-ray emission (with the angular and energy resolutions several times better than that of current γ-ray telescopes) from discrete sources; measurement of the energy spectra of Galactic and extragalactic diffuse γ-ray emission; studies of γ-ray emission from the active Sun; and measurements of fluxes of γ-ray emission and electron–positron cosmicray component, which are probably associated with the annihilation or decay of dark-matter particles. Suchkov, S. I. aut Topchiev, N. P. aut Arkhangelskaja, I. V. aut Arkhangelskiy, A. I. aut Bakaldin, A. V. aut Gusakov, Yu. V. aut Dalkarov, O. D. aut Egorov, A. E. aut Zverev, V. G. aut Kadilin, V. V. aut Leonov, A. A. aut Naumov, P. Yu. aut Runtso, M. F. aut Kheymits, M. D. aut Yurkin, Yu. T. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 80(2017), 6 vom: Nov., Seite 1141-1145 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:80 year:2017 number:6 month:11 pages:1141-1145 https://doi.org/10.1134/S1063778817060096 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 80 2017 6 11 1141-1145 |
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10.1134/S1063778817060096 doi (DE-627)OLC2049928041 (DE-He213)S1063778817060096-p DE-627 ger DE-627 rakwb eng 530 VZ Galper, A. M. verfasserin aut Precision Measurements of High-Energy Cosmic Gamma-Ray Emission with the GAMMA-400 Gamma-Ray Telescope 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2017 Abstract The GAMMA-400 γ-ray telescope installed at the Russian space observatory is intended for precision measurements in the energy range of 20 MeV–1000 GeV of γ-ray emission (with the angular and energy resolutions several times better than that of current γ-ray telescopes) from discrete sources; measurement of the energy spectra of Galactic and extragalactic diffuse γ-ray emission; studies of γ-ray emission from the active Sun; and measurements of fluxes of γ-ray emission and electron–positron cosmicray component, which are probably associated with the annihilation or decay of dark-matter particles. Suchkov, S. I. aut Topchiev, N. P. aut Arkhangelskaja, I. V. aut Arkhangelskiy, A. I. aut Bakaldin, A. V. aut Gusakov, Yu. V. aut Dalkarov, O. D. aut Egorov, A. E. aut Zverev, V. G. aut Kadilin, V. V. aut Leonov, A. A. aut Naumov, P. Yu. aut Runtso, M. F. aut Kheymits, M. D. aut Yurkin, Yu. T. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 80(2017), 6 vom: Nov., Seite 1141-1145 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:80 year:2017 number:6 month:11 pages:1141-1145 https://doi.org/10.1134/S1063778817060096 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 80 2017 6 11 1141-1145 |
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10.1134/S1063778817060096 doi (DE-627)OLC2049928041 (DE-He213)S1063778817060096-p DE-627 ger DE-627 rakwb eng 530 VZ Galper, A. M. verfasserin aut Precision Measurements of High-Energy Cosmic Gamma-Ray Emission with the GAMMA-400 Gamma-Ray Telescope 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2017 Abstract The GAMMA-400 γ-ray telescope installed at the Russian space observatory is intended for precision measurements in the energy range of 20 MeV–1000 GeV of γ-ray emission (with the angular and energy resolutions several times better than that of current γ-ray telescopes) from discrete sources; measurement of the energy spectra of Galactic and extragalactic diffuse γ-ray emission; studies of γ-ray emission from the active Sun; and measurements of fluxes of γ-ray emission and electron–positron cosmicray component, which are probably associated with the annihilation or decay of dark-matter particles. Suchkov, S. I. aut Topchiev, N. P. aut Arkhangelskaja, I. V. aut Arkhangelskiy, A. I. aut Bakaldin, A. V. aut Gusakov, Yu. V. aut Dalkarov, O. D. aut Egorov, A. E. aut Zverev, V. G. aut Kadilin, V. V. aut Leonov, A. A. aut Naumov, P. Yu. aut Runtso, M. F. aut Kheymits, M. D. aut Yurkin, Yu. T. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 80(2017), 6 vom: Nov., Seite 1141-1145 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:80 year:2017 number:6 month:11 pages:1141-1145 https://doi.org/10.1134/S1063778817060096 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 80 2017 6 11 1141-1145 |
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10.1134/S1063778817060096 doi (DE-627)OLC2049928041 (DE-He213)S1063778817060096-p DE-627 ger DE-627 rakwb eng 530 VZ Galper, A. M. verfasserin aut Precision Measurements of High-Energy Cosmic Gamma-Ray Emission with the GAMMA-400 Gamma-Ray Telescope 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2017 Abstract The GAMMA-400 γ-ray telescope installed at the Russian space observatory is intended for precision measurements in the energy range of 20 MeV–1000 GeV of γ-ray emission (with the angular and energy resolutions several times better than that of current γ-ray telescopes) from discrete sources; measurement of the energy spectra of Galactic and extragalactic diffuse γ-ray emission; studies of γ-ray emission from the active Sun; and measurements of fluxes of γ-ray emission and electron–positron cosmicray component, which are probably associated with the annihilation or decay of dark-matter particles. Suchkov, S. I. aut Topchiev, N. P. aut Arkhangelskaja, I. V. aut Arkhangelskiy, A. I. aut Bakaldin, A. V. aut Gusakov, Yu. V. aut Dalkarov, O. D. aut Egorov, A. E. aut Zverev, V. G. aut Kadilin, V. V. aut Leonov, A. A. aut Naumov, P. Yu. aut Runtso, M. F. aut Kheymits, M. D. aut Yurkin, Yu. T. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 80(2017), 6 vom: Nov., Seite 1141-1145 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:80 year:2017 number:6 month:11 pages:1141-1145 https://doi.org/10.1134/S1063778817060096 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 80 2017 6 11 1141-1145 |
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10.1134/S1063778817060096 doi (DE-627)OLC2049928041 (DE-He213)S1063778817060096-p DE-627 ger DE-627 rakwb eng 530 VZ Galper, A. M. verfasserin aut Precision Measurements of High-Energy Cosmic Gamma-Ray Emission with the GAMMA-400 Gamma-Ray Telescope 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2017 Abstract The GAMMA-400 γ-ray telescope installed at the Russian space observatory is intended for precision measurements in the energy range of 20 MeV–1000 GeV of γ-ray emission (with the angular and energy resolutions several times better than that of current γ-ray telescopes) from discrete sources; measurement of the energy spectra of Galactic and extragalactic diffuse γ-ray emission; studies of γ-ray emission from the active Sun; and measurements of fluxes of γ-ray emission and electron–positron cosmicray component, which are probably associated with the annihilation or decay of dark-matter particles. Suchkov, S. I. aut Topchiev, N. P. aut Arkhangelskaja, I. V. aut Arkhangelskiy, A. I. aut Bakaldin, A. V. aut Gusakov, Yu. V. aut Dalkarov, O. D. aut Egorov, A. E. aut Zverev, V. G. aut Kadilin, V. V. aut Leonov, A. A. aut Naumov, P. Yu. aut Runtso, M. F. aut Kheymits, M. D. aut Yurkin, Yu. T. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 80(2017), 6 vom: Nov., Seite 1141-1145 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:80 year:2017 number:6 month:11 pages:1141-1145 https://doi.org/10.1134/S1063778817060096 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 80 2017 6 11 1141-1145 |
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precision measurements of high-energy cosmic gamma-ray emission with the gamma-400 gamma-ray telescope |
| title_auth |
Precision Measurements of High-Energy Cosmic Gamma-Ray Emission with the GAMMA-400 Gamma-Ray Telescope |
| abstract |
Abstract The GAMMA-400 γ-ray telescope installed at the Russian space observatory is intended for precision measurements in the energy range of 20 MeV–1000 GeV of γ-ray emission (with the angular and energy resolutions several times better than that of current γ-ray telescopes) from discrete sources; measurement of the energy spectra of Galactic and extragalactic diffuse γ-ray emission; studies of γ-ray emission from the active Sun; and measurements of fluxes of γ-ray emission and electron–positron cosmicray component, which are probably associated with the annihilation or decay of dark-matter particles. © Pleiades Publishing, Ltd. 2017 |
| abstractGer |
Abstract The GAMMA-400 γ-ray telescope installed at the Russian space observatory is intended for precision measurements in the energy range of 20 MeV–1000 GeV of γ-ray emission (with the angular and energy resolutions several times better than that of current γ-ray telescopes) from discrete sources; measurement of the energy spectra of Galactic and extragalactic diffuse γ-ray emission; studies of γ-ray emission from the active Sun; and measurements of fluxes of γ-ray emission and electron–positron cosmicray component, which are probably associated with the annihilation or decay of dark-matter particles. © Pleiades Publishing, Ltd. 2017 |
| abstract_unstemmed |
Abstract The GAMMA-400 γ-ray telescope installed at the Russian space observatory is intended for precision measurements in the energy range of 20 MeV–1000 GeV of γ-ray emission (with the angular and energy resolutions several times better than that of current γ-ray telescopes) from discrete sources; measurement of the energy spectra of Galactic and extragalactic diffuse γ-ray emission; studies of γ-ray emission from the active Sun; and measurements of fluxes of γ-ray emission and electron–positron cosmicray component, which are probably associated with the annihilation or decay of dark-matter particles. © Pleiades Publishing, Ltd. 2017 |
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GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 |
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6 |
| title_short |
Precision Measurements of High-Energy Cosmic Gamma-Ray Emission with the GAMMA-400 Gamma-Ray Telescope |
| url |
https://doi.org/10.1134/S1063778817060096 |
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| author2 |
Suchkov, S. I. Topchiev, N. P. Arkhangelskaja, I. V. Arkhangelskiy, A. I. Bakaldin, A. V. Gusakov, Yu. V. Dalkarov, O. D. Egorov, A. E. Zverev, V. G. Kadilin, V. V. Leonov, A. A. Naumov, P. Yu Runtso, M. F. Kheymits, M. D. Yurkin, Yu. T. |
| author2Str |
Suchkov, S. I. Topchiev, N. P. Arkhangelskaja, I. V. Arkhangelskiy, A. I. Bakaldin, A. V. Gusakov, Yu. V. Dalkarov, O. D. Egorov, A. E. Zverev, V. G. Kadilin, V. V. Leonov, A. A. Naumov, P. Yu Runtso, M. F. Kheymits, M. D. Yurkin, Yu. T. |
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131188437 |
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| doi_str |
10.1134/S1063778817060096 |
| up_date |
2024-07-04T00:31:54.287Z |
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