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J-GLOBAL ID：201802253817080863   整理番号：18A2070597

MeV-GeVガンマ線天体物理学のためのE-ASTROGAM A宇宙ミッションによる科学【JST・京大機械翻訳】

Science with e-ASTROGAM A space mission for MeV-GeV gamma-ray astrophysics

著者 (120件)： De Angelis A. (Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova, Italy) ,  De Angelis A. (INAF - Osservatorio Astronomico di Padova, I-35122, Padova, Italy) ,  De Angelis A. (Dipartimento di Matematica, Informatica e Fisica, Universita di Udine, I-33100 Udine, Italy) ,  De Angelis A. (Laboratorio de Instrumentacao e Particulas and Instituto Superior Tecnico, Lisboa, Portugal) ,  Tatischeff V. (CSNSM, CNRS and University of Paris Sud, F-91405, Orsay, France) ,  Grenier I.A. (Laboratoire AIM, CEA-IRFU/CNRS/Universite Paris Diderot, C.E.A. Saclay, France) ,  McEnery J. (NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA) ,  Mallamaci M. (Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova, Italy) ,  Tavani M. (INAF/IAPS, via del Fosso del Cavaliere 100, I-00133, Roma, Italy) ,  Tavani M. (University of Roma “Tor Vergata”, I-00133, Roma, Italy) ,  Tavani M. (Istituto Nazionale di Fisica Nucleare, Sezione di Roma “Tor Vergata”, I-00133 Roma, Italy) ,  Oberlack U. (Institute of Physics and PRISMA Excellence Cluster, Johannes Gutenberg University Mainz, 55099 Mainz, Germany) ,  Hanlon L. (School of Physics, University College Dublin, Ireland) ,  Walter R. (University of Geneva, Switzerland) ,  Argan A. (INAF Headquarters, Viale del Parco Mellini, 84, I-00136, Roma, Italy) ,  Von Ballmoos P. (IRAP Toulouse, 9 av. du Colonel-Roche - BP 44 346, F-31028 Toulouse Cedex 4, France) ,  Bulgarelli A. (INAF/OAS-Bologna, Via Gobetti 93, I-40129 Bologna, Italy) ,  Bykov A. (Ioffe Institute, St. Petersburg 194021, Russia) ,  Hernanz M. (Institute of Space Sciences (CSIC-IEEC), Campus UAB, C/Can Magrans s/n, 08193 Cerdanyola del Valles (Barcelona), Spain) ,  Kanbach G. (Max-Planck-Institut fuer Extraterrestrische Physik, Postfach 1312, 85741 Garching, Germany) ,  Kuvvetli I. (DTU Space, National Space Institute, Technical University of Denmark, Kgs. Lyngby, Denmark) ,  Pearce M. (Physics Department, Royal Institute of Technology (KTH), 10691 Stockholm, Sweden) ,  Zdziarski A. (Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, PL-00-716 Warszawa, Poland) ,  Conrad J. (Oskar Klein Centre for Cosmoparticle Physics Fysikum, Stockholm University, AlbaNova University Centre, SE-10961, Stockholm, Sweden) ,  Ghisellini G. (INAF - Osservatorio Astronomico di Brera, I-23807 Merate, Italy) ,  Harding A. (NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA) ,  Isern J. (ICE (CSIC-IEEC), Campus UAB, Carrer Can Magrans s/n, E-08193 Cerdanyola del Valles, Barcelona, Spain) ,  Leising M. (Department of Physics and Astronomy, Clemson University, Clemson, SC 29634, USA) ,  Longo F. (Dipartimento di Fisica, Universita di Trieste, I-34127 Trieste, Italy) ,  Longo F. (Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I-34127 Trieste, Italy) ,  Madejski G. (W.W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA, 94305, USA) ,  Martinez M. (IFAE-BIST, Edifici Cn. Universitat Autonoma de Barcelona, E-08193 Bellaterra, Spain) ,  Mazziotta M.N. (Istituto Nazionale di Fisica Nucleare, Sezione di Bari, I-70126, Bari, Italy) ,  Paredes J.M. (Departament de Fisica Quantica i Astrofisica, Institut de Ciencies del Cosmos (ICCUB), Universitat de Barcelona, IEEC-UB, Marti i Franques 1, E08028 Barcelona, Spain) ,  Pohl M. (Institute of Physics and Astronomy, University of Potsdam, 14476 Potsdam, Germany) ,  Rando R. (Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova, Italy) ,  Rando R. (Dipartimento di Fisica e Astronomia “G. Galilei”, Universita di Padova, I-35131 Padova, Italy) ,  Razzano M. (Istituto Nazionale di Fisica Nucleare, I-56127, Pisa, Italy) ,  Razzano M. (Dipartimento di Fisica “E. Fermi”, Universita di Pisa, I-56127, Pisa, Italy) ,  Aboudan A. (Dipartimento di Fisica e Astronomia “G. Galilei”, Universita di Padova, I-35131 Padova, Italy) ,  Aboudan A. (INAF - Osservatorio Astronomico di Padova, I-35122, Padova, Italy) ,  Ackermann M. (Deutsches Elektronen Synchrotron (DESY), Platanenallee 6, D-15738, Zeuthen, Germany) ,  Addazi A. (Center for Field Theory and Particle Physics & Department of Physics, Fudan University, 200433 Shanghai, China) ,  Ajello M. (Department of Physics and Astronomy, Clemson University, Clemson, SC 29634, USA) ,  Albertus C. (Department of Fundamental Physics and IUFFyM University of Salamanca, Plaza de la Merced s/n 37008, Spain) ,  Alvarez J.M. (Spanish Center for Pulsed Lasers (CLPU), M5 Bldg., Science Park, Villamayor, Salamanca, Spain) ,  Ambrosi G. (Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123, Perugia, Italy) ,  Anton S. (CIDMA, Dep. de Fisica, Univ. de Aveiro, Campus de Santiago, 3810-193 Aveiro, Portugal) ,  Anton S. (Inst. Telecomunicacoees, Campus de Santiago, 3810-193 Aveiro, Portugal) ,  Antonelli L.A. (Space Science Data Center, Agenzia Spaziale Italiana, I-00133, Roma, Italy) ,  Babic A. (Faculty of Electrical Engineering and Computing, University of Zagreb, Croatia) ,  Baibussinov B. (Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova, Italy) ,  Balbo M. (University of Geneva, Switzerland) ,  Baldini L. (Istituto Nazionale di Fisica Nucleare, I-56127, Pisa, Italy) ,  Baldini L. (Dipartimento di Fisica “E. Fermi”, Universita di Pisa, I-56127, Pisa, Italy) ,  Balman S. (Department of Physics, Middle East Technical University, Ankara, Turkey) ,  Bambi C. (Center for Field Theory and Particle Physics & Department of Physics, Fudan University, 200433 Shanghai, China) ,  Bambi C. (Eberhard-Karls Universitat Tuebingen, 72076 Tuebingen, Germany) ,  Barres de Almeida U. (Brazilian Center for Research in Physics, Rio de Janeiro, Brazil) ,  Barrio J.A. (Unidad de Particulars y Cosmologia (UPARCOS), Universidad Complutense, E-28040 Madrid, Spain) ,  Bartels R. (GRAPPA and Institute of Physics, University of Amsterdam, Science Park 904, 1098XH Amsterdam, the Netherlands) ,  Bastieri D. (Dipartimento di Fisica e Astronomia “G. Galilei”, Universita di Padova, I-35131 Padova, Italy) ,  Bastieri D. (Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova, Italy) ,  Bastieri D. (Center for Astrophysics, Guangzhou University, Guangzhou 510006, China) ,  Bednarek W. (Department of Astrophysics, University of Lodz, ul. Pomorska 149/153, 90-236 Lodz, Poland) ,  Bernard D. (LLR, Ecole Polytechnique, CNRS/IN2P3, 91128 Palaiseau, France) ,  Bernardini E. (Institut fuer Physik, Humboldt-Universitaet zu Berlin, D-12489 Berlin, Germany) ,  Bernardini E. (Deutsches Elektronen Synchrotron (DESY), Platanenallee 6, D-15738, Zeuthen, Germany) ,  Bernasconi T. (University of Geneva, Switzerland) ,  Bertucci B. (Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123, Perugia, Italy) ,  Bertucci B. (Universita di Perugia, I-06123 Perugia, Italy) ,  Biland A. (ETH, Zuerich, Switzerland) ,  Bissaldi E. (Dipartimento di Fisica “M. Merlin” dell’Universita e del Politecnico di Bari, I-70126, Bari, Italy) ,  Bissaldi E. (Istituto Nazionale di Fisica Nucleare, Sezione di Bari, I-70126, Bari, Italy) ,  Boettcher M. (North-West University, Potchefstroom, South Africa) ,  Bonvicini V. (Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I-34127 Trieste, Italy) ,  Bosch-Ramon V. (Departament de Fisica Quantica i Astrofisica, Institut de Ciencies del Cosmos (ICCUB), Universitat de Barcelona, IEEC-UB, Marti i Franques 1, E08028 Barcelona, Spain) ,  Bottacini E. (Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova, Italy) ,  Bottacini E. (Dipartimento di Fisica e Astronomia “G. Galilei”, Universita di Padova, I-35131 Padova, Italy) ,  Bozhilov V. (Faculty of Physics, University of Sofia “St. Kl. Ohridski”, Sofia 1164, Bulgaria) ,  Bretz T. (RWTH Aachen University, D-52074 Aachen, Germany) ,  Branchesi M. ,  Branchesi M. ,  Brdar V. ,  Bringmann T. ,  Brogna A. (Institute of Physics and PRISMA Excellence Cluster, Johannes Gutenberg University Mainz, 55099 Mainz, Germany) ,  Budtz Jorgensen C. (DTU Space, National Space Institute, Technical University of Denmark, Kgs. Lyngby, Denmark) ,  Busetto G. (Dipartimento di Fisica e Astronomia “G. Galilei”, Universita di Padova, I-35131 Padova, Italy) ,  Buson S. (NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA) ,  Busso M. (Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123, Perugia, Italy) ,  Busso M. (Universita di Perugia, I-06123 Perugia, Italy) ,  Caccianiga A. (INAF - Osservatorio Astronomico di Brera, I-23807 Merate, Italy) ,  Camera S. ,  Camera S. ,  Camera S. ,  Camera S. ,  Campana R. (INAF/OAS-Bologna, Via Gobetti 93, I-40129 Bologna, Italy) ,  Caraveo P. ,  Cardillo M. (INAF/IAPS, via del Fosso del Cavaliere 100, I-00133, Roma, Italy) ,  Carlson P. (Physics Department, Royal Institute of Technology (KTH), 10691 Stockholm, Sweden) ,  Celestin S. ,  Cermeno M. (Department of Fundamental Physics and IUFFyM University of Salamanca, Plaza de la Merced s/n 37008, Spain) ,  Chen A. ,  Cheung C.C. ,  Churazov E. ,  Churazov E. ,  Ciprini S. (Space Science Data Center, Agenzia Spaziale Italiana, I-00133, Roma, Italy) ,  Ciprini S. (Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123, Perugia, Italy) ,  Coc A. (CSNSM, CNRS and University of Paris Sud, F-91405, Orsay, France) ,  Colafrancesco S. ,  Coleiro A. ,  Coleiro A. ,  Collmar W. ,  Coppi P. ,  Curado da Silva R. ,  Cutini S. (Space Science Data Center, Agenzia Spaziale Italiana, I-00133, Roma, Italy) ,  Cutini S. (Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123, Perugia, Italy) ,  D’Ammando F. ,  De Lotto B. ,  de Martino D.
資料名： Journal of High Energy Astrophysics  (Journal of High Energy Astrophysics)
巻： 19  ページ： 1-106  発行年： 2018年 
JST資料番号： W2992A  ISSN： 2214-4048  資料種別： 逐次刊行物 (A)
記事区分： 原著論文  発行国： オランダ (NLD)  言語： 英語 (EN)

抄録/ポイント： e-ASTROGAM(「強化ASTROGAM」)は,0.3MeVから3GeVまでの光子エネルギー範囲での非熱的Uni逆の研究に専用の,シリコントラッカー,熱量計,および反同時計数システムで構成されるブレークスルー観測空間ミッションであり,低エネルギー限界はトラッカーに対して150keV,熱量検出に対して30keVと低いエネルギーに押すことができる。ミッションは,先例のない感度,角度およびエネルギー分解能を有する先進的な空間証明検出器技術に基づいている。MeV-GeV領域における性能のおかげで,本質的に,e-ASTROGAMは,非熱的Universeに関する新しい窓を開き,最も強力な銀河と銀河外源の先駆的観測を行い,それらの相対論的流出の性質と周辺への影響を解明した。MeVエネルギー範囲における線感度は,以前の生成装置よりも1~2桁良いので,e-ASTROGAMは,超新星爆発の理解と我々の銀河の化学進化に対する重要な同位体の起源を決定するであろう。ミッションは,LIGO-Virgo-GEO600-KAGRA,SKA,ALMA,E-ELT,TMT,LSST,JWST,Athena,CTA,IceCube,KM3NeT,LISAのような強力な観測所に相補的な,広い天文学的コミュニティへの重要な関心のユニークなデータを提供する。Copyright 2018 Elsevier B.V., Amsterdam. All rights reserved. Translated from English into Japanese by JST.【JST・京大機械翻訳】

シソーラス用語： *γ線 ,  超新星爆発 ,  *宇宙空間 ,  コミュニティ ,  化学進化 ,  エネルギー ,  同位体 ,  熱量 ,  相対論 ,  検出器 ,  エネルギー分解能 ,  *宇宙物理学
準シソーラス用語： LIGO ,  再生器 ,  低エネルギー , 【Automatic Indexing@JST】

分類 (2件)： 宇宙線起源  (DB02020Q) ,  宇宙線・天体物理観測技術  (DB01000N)

タイトルに関連する用語 (5件)： ガンマ線 ,  天体物理学 ,  宇宙 ,  ミッション ,  科学