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http://hdl.handle.net/10261/170333
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dc.contributor.author | Barret, Didier | - |
dc.contributor.author | Nandra, K. | - |
dc.contributor.author | Barcons, Xavier | - |
dc.contributor.author | Fabian, Andrew C. | - |
dc.contributor.author | Herder, J. W. den | - |
dc.contributor.author | Piro, Luigi | - |
dc.contributor.author | Watson, Mike | - |
dc.contributor.author | Aird, James | - |
dc.contributor.author | Branduardi-Raymont, G. | - |
dc.contributor.author | Cappi, Massimo | - |
dc.contributor.author | Carrera, Francisco J. | - |
dc.contributor.author | Comastri, A. | - |
dc.contributor.author | Costantini, E. | - |
dc.contributor.author | Croston, J. | - |
dc.contributor.author | Decourchelle, A. | - |
dc.contributor.author | Done, Chris | - |
dc.contributor.author | Dovciak, M. | - |
dc.contributor.author | Ettori, S. | - |
dc.contributor.author | Finoguenov, Alexis | - |
dc.contributor.author | Georgakakis, Antonis | - |
dc.contributor.author | Jonker, P. | - |
dc.contributor.author | Kaastra, Jelle | - |
dc.contributor.author | Matt, Giorgio | - |
dc.contributor.author | Motch, Christian | - |
dc.contributor.author | O'Brien, P. | - |
dc.contributor.author | Pareschi, G. | - |
dc.contributor.author | Pointecouteau, E. | - |
dc.contributor.author | Pratt, G.W. | - |
dc.contributor.author | Rauw, G. | - |
dc.contributor.author | Reiprich, T. | - |
dc.contributor.author | Sanders, J. | - |
dc.contributor.author | Sciortino, Salvatore | - |
dc.contributor.author | Willingale, Richard | - |
dc.contributor.author | Wilms, Jörn | - |
dc.date.accessioned | 2018-09-28T08:43:13Z | - |
dc.date.available | 2018-09-28T08:43:13Z | - |
dc.date.issued | 2013 | - |
dc.identifier.citation | Annual Meeting of the French Society of Astronomy and Astrophysics (2013) | - |
dc.identifier.uri | http://hdl.handle.net/10261/170333 | - |
dc.description | Trabajo presentado al Annual Meeting of the French Society of Astronomy and Astrophysics (SF2A), celebrado en Montpellier del 4 al 7 de junio de 2013. | - |
dc.description.abstract | The Advanced Telescope for High-energy Astrophysics (Athena+) is being proposed to ESA as the L2 mission (for a launch in 2028) and is specifically designed to answer two of the most pressing questions for astrophysics in the forthcoming decade: How did ordinary matter assemble into the large scale structures we see today? and how do black holes grow and shape the Universe? For addressing these two issues, Athena+ will provide transformational capabilities in terms of angular resolution, effective area, spectral resolution, grasp, that will make it the most powerful X-ray observatory ever flown. Such an observatory, when opened to the astronomical community, will be used for virtually all classes of astrophysical objects, from high-z gamma-ray bursts to the closest planets in our solar neighborhood. In this paper, we briefly review the core science objectives of Athena+, present the science requirements and the foreseen implementation of the mission, and illustrate its transformational capabilities compared to existing facilities. | - |
dc.relation.isversionof | Publisher's version | - |
dc.rights | openAccess | - |
dc.title | Athena+: the first deep universe X-ray observatory | - |
dc.type | comunicación de congreso | - |
dc.date.updated | 2018-09-28T08:43:14Z | - |
dc.description.version | Peer Reviewed | - |
dc.language.rfc3066 | eng | - |
dc.relation.csic | Sí | - |
dc.type.coar | http://purl.org/coar/resource_type/c_5794 | es_ES |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.openairetype | comunicación de congreso | - |
item.grantfulltext | open | - |
Aparece en las colecciones: | (IFCA) Comunicaciones congresos |
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athenamas.pdf | 2,84 MB | Adobe PDF | Visualizar/Abrir |
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