{ "id": "1912.04615", "version": "v1", "published": "2019-12-10T10:21:29.000Z", "updated": "2019-12-10T10:21:29.000Z", "title": "The Athena space X-ray Observatory and the astrophysics of hot plasma", "authors": [ "Didier Barret", "Anne Decourchelle", "Andy Fabian", "Matteo Guainazzi", "Kirpal Nandra", "Randall Smith", "Jan-Willem den Herder" ], "comment": "12 pages, 9 figures, Proceedings of the XMM-Newton 2019 science workshop \"Astrophysics of hot plasma in extended X -ray sources\", accepted for publication in Astronomische Nachrichten", "categories": [ "astro-ph.IM", "astro-ph.GA", "astro-ph.HE" ], "abstract": "The properties (temperature, density, chemical composition, velocity) of hot astrophysical plasma and the physical processes affecting them (heating/cooling, turbulence, shocks, acceleration) can be probed by high resolution X-ray spectroscopy, to be complemented by high spatial resolution imaging. The paper presents a status of the ESA's Advanced Telescope for High Energy Astrophysics (Athena) mission, particularly focusing on the science performance of its two focal plane instruments for the studies of extended X-ray sources: the Wide Field Imager (WFI) and the X-ray Integral Field Unit (X-IFU). This paper then provides a brief summary of the breakthroughs expected with Athena on the astrophysics of hot plasma, building on the vast heritage of the discoveries and revolutionary results obtained by Chandra and XMM-Newton in this field. As of November 12th, 2019, Athena successfully concluded its feasibility study, and has since then moved into the definition phase, with a launch date scheduled in the early 2030s.", "revisions": [ { "version": "v1", "updated": "2019-12-10T10:21:29.000Z" } ], "analyses": { "keywords": [ "athena space x-ray observatory", "hot plasma", "x-ray integral field unit", "high resolution x-ray spectroscopy", "high spatial resolution" ], "note": { "typesetting": "TeX", "pages": 12, "language": "en", "license": "arXiv", "status": "editable" } } }