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dc.contributor.authorBarret, Didier-
dc.contributor.authorNandra, K.-
dc.contributor.authorBarcons, Xavier-
dc.contributor.authorFabian, Andrew C.-
dc.contributor.authorHerder, J. W. den-
dc.contributor.authorPiro, Luigi-
dc.contributor.authorWatson, Mike-
dc.contributor.authorAird, James-
dc.contributor.authorBranduardi-Raymont, G.-
dc.contributor.authorCappi, Massimo-
dc.contributor.authorCarrera, Francisco J.-
dc.contributor.authorComastri, A.-
dc.contributor.authorCostantini, E.-
dc.contributor.authorCroston, J.-
dc.contributor.authorDecourchelle, A.-
dc.contributor.authorDone, Chris-
dc.contributor.authorDovciak, M.-
dc.contributor.authorEttori, S.-
dc.contributor.authorFinoguenov, Alexis-
dc.contributor.authorGeorgakakis, Antonis-
dc.contributor.authorJonker, P.-
dc.contributor.authorKaastra, Jelle-
dc.contributor.authorMatt, Giorgio-
dc.contributor.authorMotch, Christian-
dc.contributor.authorO'Brien, P.-
dc.contributor.authorPareschi, G.-
dc.contributor.authorPointecouteau, E.-
dc.contributor.authorPratt, G.W.-
dc.contributor.authorRauw, G.-
dc.contributor.authorReiprich, T.-
dc.contributor.authorSanders, J.-
dc.contributor.authorSciortino, Salvatore-
dc.contributor.authorWillingale, Richard-
dc.contributor.authorWilms, Jörn-
dc.date.accessioned2018-09-28T08:43:13Z-
dc.date.available2018-09-28T08:43:13Z-
dc.date.issued2013-
dc.identifier.citationAnnual Meeting of the French Society of Astronomy and Astrophysics (2013)-
dc.identifier.urihttp://hdl.handle.net/10261/170333-
dc.descriptionTrabajo 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.abstractThe 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.isversionofPublisher's version-
dc.rightsopenAccess-
dc.titleAthena+: the first deep universe X-ray observatory-
dc.typecomunicación de congreso-
dc.date.updated2018-09-28T08:43:14Z-
dc.description.versionPeer Reviewed-
dc.language.rfc3066eng-
dc.relation.csic-
dc.type.coarhttp://purl.org/coar/resource_type/c_5794es_ES
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
item.cerifentitytypePublications-
item.openairetypecomunicación de congreso-
item.grantfulltextopen-
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