GAMMA-400 Gamma-Ray Observations in the GeV and TeV Energy Range
The future space-based GAMMA-400 -ray telescope will operate onboard the Russian astrophysical observatory in a highly elliptic orbit during 7 years. Observing -ray sources from Galactic plane, -ray bursts, -ray diffuse emission, rays from the Sun, and rays from dark matter particles will be perform...
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| Veröffentlicht in: | Physics of atomic nuclei 2021-11, Vol.84 (6), p.1053-1058 |
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| creator | Topchiev, N. P. Galper, A. M. Arkhangelskaja, I. V. Arkhangelskiy, A. I. Bakaldin, A. V. Cherniy, R. A. Chernysheva, I. V. Dalkarov, O. D. Egorov, A. E. Kheymits, M. D. Korotkov, M. G. Leonov, A. A. Malinin, A. G. Mikhailov, V. V. Minaev, P. Yu Pappe, N. Yu Runtso, M. F. Smirnov, A. I. Stozhkov, Yu. I. Suchkov, S. I. Yurkin, Yu. T. |
| description | The future space-based GAMMA-400
-ray telescope will operate onboard the Russian astrophysical observatory in a highly elliptic orbit during 7 years. Observing
-ray sources from Galactic plane,
-ray bursts,
-ray diffuse emission,
rays from the Sun, and
rays from dark matter particles will be performed uninterruptedly for a long time (
100 days) in point-source mode in contrast to scanning mode for Fermi-LAT and other space- and ground-based instruments. GAMMA-400 will measure
rays in the energy range from
20 MeV to several TeV units, have the unprecedented angular (
at
GeV) and energy (
at
GeV) resolutions better than for Fermi-LAT, as well as ground-based
-ray facilities, by a factor of 5–10, and perfectly separate
rays from cosmic-ray background. |
| doi_str_mv | 10.1134/S106377882113038X |
| format | Article |
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-ray telescope will operate onboard the Russian astrophysical observatory in a highly elliptic orbit during 7 years. Observing
-ray sources from Galactic plane,
-ray bursts,
-ray diffuse emission,
rays from the Sun, and
rays from dark matter particles will be performed uninterruptedly for a long time (
100 days) in point-source mode in contrast to scanning mode for Fermi-LAT and other space- and ground-based instruments. GAMMA-400 will measure
rays in the energy range from
20 MeV to several TeV units, have the unprecedented angular (
at
GeV) and energy (
at
GeV) resolutions better than for Fermi-LAT, as well as ground-based
-ray facilities, by a factor of 5–10, and perfectly separate
rays from cosmic-ray background.</description><identifier>ISSN: 1063-7788</identifier><identifier>EISSN: 1562-692X</identifier><identifier>DOI: 10.1134/S106377882113038X</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Cosmic rays ; Dark matter ; Dark matter (Astronomy) ; Elementary Particles and Fields/Experiment ; Gamma rays ; Particle and Nuclear Physics ; Physics ; Physics and Astronomy ; Point sources ; Telescope</subject><ispartof>Physics of atomic nuclei, 2021-11, Vol.84 (6), p.1053-1058</ispartof><rights>Pleiades Publishing, Ltd. 2021</rights><rights>COPYRIGHT 2021 Springer</rights><rights>Pleiades Publishing, Ltd. 2021.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c389t-4a419d242764d72cbb3b10e3146284a73c21cd94db6cf81c75cf125f981760c03</citedby><cites>FETCH-LOGICAL-c389t-4a419d242764d72cbb3b10e3146284a73c21cd94db6cf81c75cf125f981760c03</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S106377882113038X$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S106377882113038X$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Topchiev, N. P.</creatorcontrib><creatorcontrib>Galper, A. M.</creatorcontrib><creatorcontrib>Arkhangelskaja, I. V.</creatorcontrib><creatorcontrib>Arkhangelskiy, A. I.</creatorcontrib><creatorcontrib>Bakaldin, A. V.</creatorcontrib><creatorcontrib>Cherniy, R. A.</creatorcontrib><creatorcontrib>Chernysheva, I. V.</creatorcontrib><creatorcontrib>Dalkarov, O. D.</creatorcontrib><creatorcontrib>Egorov, A. E.</creatorcontrib><creatorcontrib>Kheymits, M. D.</creatorcontrib><creatorcontrib>Korotkov, M. G.</creatorcontrib><creatorcontrib>Leonov, A. A.</creatorcontrib><creatorcontrib>Malinin, A. G.</creatorcontrib><creatorcontrib>Mikhailov, V. V.</creatorcontrib><creatorcontrib>Minaev, P. Yu</creatorcontrib><creatorcontrib>Pappe, N. Yu</creatorcontrib><creatorcontrib>Runtso, M. F.</creatorcontrib><creatorcontrib>Smirnov, A. I.</creatorcontrib><creatorcontrib>Stozhkov, Yu. I.</creatorcontrib><creatorcontrib>Suchkov, S. I.</creatorcontrib><creatorcontrib>Yurkin, Yu. T.</creatorcontrib><title>GAMMA-400 Gamma-Ray Observations in the GeV and TeV Energy Range</title><title>Physics of atomic nuclei</title><addtitle>Phys. Atom. Nuclei</addtitle><description>The future space-based GAMMA-400
-ray telescope will operate onboard the Russian astrophysical observatory in a highly elliptic orbit during 7 years. Observing
-ray sources from Galactic plane,
-ray bursts,
-ray diffuse emission,
rays from the Sun, and
rays from dark matter particles will be performed uninterruptedly for a long time (
100 days) in point-source mode in contrast to scanning mode for Fermi-LAT and other space- and ground-based instruments. GAMMA-400 will measure
rays in the energy range from
20 MeV to several TeV units, have the unprecedented angular (
at
GeV) and energy (
at
GeV) resolutions better than for Fermi-LAT, as well as ground-based
-ray facilities, by a factor of 5–10, and perfectly separate
rays from cosmic-ray background.</description><subject>Cosmic rays</subject><subject>Dark matter</subject><subject>Dark matter (Astronomy)</subject><subject>Elementary Particles and Fields/Experiment</subject><subject>Gamma rays</subject><subject>Particle and Nuclear Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Point sources</subject><subject>Telescope</subject><issn>1063-7788</issn><issn>1562-692X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNp1kUFLwzAUgIsoOKc_wFvBk4fOvCRN05tlaB1sDLYpu5U0TWvHms6kE_fvzaggQySHl-R930t4z_NuAY0ACH1YAmIkijjH7ogIX595AwgZDliM1-du79LBMX_pXVm7QQiAh2jgPabJbJYEFCE_FU0jgoU4-PPcKvMpurrV1q-1370rP1VvvtCFv3LxSStTHfyF0JW69i5KsbXq5icOvdfnp9X4JZjO08k4mQaS8LgLqKAQF5jiiNEiwjLPSQ5IEaAMcyoiIjHIIqZFzmTJQUahLAGHZcwhYkgiMvTu-ro7037sle2yTbs32j2ZYQYhAUxj7KhRT1Viq7Jal21nhHSrUE0tW63K2t0nzPUpBo6Owv2J4JhOfXWV2FubTZaLUxZ6VprWWqPKbGfqRphDBig7TiH7MwXn4N6xjnXtMr_f_l_6BiO9g9A</recordid><startdate>20211101</startdate><enddate>20211101</enddate><creator>Topchiev, N. 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T.</creator><general>Pleiades Publishing</general><general>Springer</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>ISR</scope></search><sort><creationdate>20211101</creationdate><title>GAMMA-400 Gamma-Ray Observations in the GeV and TeV Energy Range</title><author>Topchiev, N. P. ; Galper, A. M. ; Arkhangelskaja, I. V. ; Arkhangelskiy, A. I. ; Bakaldin, A. V. ; Cherniy, R. A. ; Chernysheva, I. V. ; Dalkarov, O. D. ; Egorov, A. E. ; Kheymits, M. D. ; Korotkov, M. G. ; Leonov, A. A. ; Malinin, A. G. ; Mikhailov, V. V. ; Minaev, P. Yu ; Pappe, N. Yu ; Runtso, M. F. ; Smirnov, A. I. ; Stozhkov, Yu. I. ; Suchkov, S. I. ; Yurkin, Yu. 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A.</creatorcontrib><creatorcontrib>Chernysheva, I. V.</creatorcontrib><creatorcontrib>Dalkarov, O. D.</creatorcontrib><creatorcontrib>Egorov, A. E.</creatorcontrib><creatorcontrib>Kheymits, M. D.</creatorcontrib><creatorcontrib>Korotkov, M. G.</creatorcontrib><creatorcontrib>Leonov, A. A.</creatorcontrib><creatorcontrib>Malinin, A. G.</creatorcontrib><creatorcontrib>Mikhailov, V. V.</creatorcontrib><creatorcontrib>Minaev, P. Yu</creatorcontrib><creatorcontrib>Pappe, N. Yu</creatorcontrib><creatorcontrib>Runtso, M. F.</creatorcontrib><creatorcontrib>Smirnov, A. I.</creatorcontrib><creatorcontrib>Stozhkov, Yu. I.</creatorcontrib><creatorcontrib>Suchkov, S. I.</creatorcontrib><creatorcontrib>Yurkin, Yu. T.</creatorcontrib><collection>CrossRef</collection><collection>Gale In Context: Science</collection><jtitle>Physics of atomic nuclei</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Topchiev, N. P.</au><au>Galper, A. M.</au><au>Arkhangelskaja, I. V.</au><au>Arkhangelskiy, A. I.</au><au>Bakaldin, A. V.</au><au>Cherniy, R. A.</au><au>Chernysheva, I. V.</au><au>Dalkarov, O. D.</au><au>Egorov, A. E.</au><au>Kheymits, M. D.</au><au>Korotkov, M. G.</au><au>Leonov, A. A.</au><au>Malinin, A. G.</au><au>Mikhailov, V. V.</au><au>Minaev, P. Yu</au><au>Pappe, N. Yu</au><au>Runtso, M. F.</au><au>Smirnov, A. I.</au><au>Stozhkov, Yu. I.</au><au>Suchkov, S. I.</au><au>Yurkin, Yu. T.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>GAMMA-400 Gamma-Ray Observations in the GeV and TeV Energy Range</atitle><jtitle>Physics of atomic nuclei</jtitle><stitle>Phys. Atom. Nuclei</stitle><date>2021-11-01</date><risdate>2021</risdate><volume>84</volume><issue>6</issue><spage>1053</spage><epage>1058</epage><pages>1053-1058</pages><issn>1063-7788</issn><eissn>1562-692X</eissn><abstract>The future space-based GAMMA-400
-ray telescope will operate onboard the Russian astrophysical observatory in a highly elliptic orbit during 7 years. Observing
-ray sources from Galactic plane,
-ray bursts,
-ray diffuse emission,
rays from the Sun, and
rays from dark matter particles will be performed uninterruptedly for a long time (
100 days) in point-source mode in contrast to scanning mode for Fermi-LAT and other space- and ground-based instruments. GAMMA-400 will measure
rays in the energy range from
20 MeV to several TeV units, have the unprecedented angular (
at
GeV) and energy (
at
GeV) resolutions better than for Fermi-LAT, as well as ground-based
-ray facilities, by a factor of 5–10, and perfectly separate
rays from cosmic-ray background.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S106377882113038X</doi><tpages>6</tpages></addata></record> |
| fulltext | fulltext |
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| ispartof | Physics of atomic nuclei, 2021-11, Vol.84 (6), p.1053-1058 |
| issn | 1063-7788 1562-692X |
| language | eng |
| recordid | cdi_proquest_journals_2615312492 |
| source | SpringerLink Journals |
| subjects | Cosmic rays Dark matter Dark matter (Astronomy) Elementary Particles and Fields/Experiment Gamma rays Particle and Nuclear Physics Physics Physics and Astronomy Point sources Telescope |
| title | GAMMA-400 Gamma-Ray Observations in the GeV and TeV Energy Range |
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