{
  "id": "1611.06909",
  "version": "v1",
  "published": "2016-11-21T17:24:24.000Z",
  "updated": "2016-11-21T17:24:24.000Z",
  "title": "The Future of X-ray Reverberation from AGN",
  "authors": [
    "A. C. Fabian",
    "W. N. Alston",
    "E. M. Cackett",
    "E. Kara",
    "P. Uttley",
    "D. R. Wilkins"
  ],
  "comment": "5 pages, 5 figures for publication in Astronomische Nachrichten as part of the proceedings of the workshop \"XMM-Newton: The Next Decade\"",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "XMM-Newton is capable of making a transformational advance in our understanding of how luminous accreting black holes work, by dedicating about 10 per cent of future observing time to long observations, of order Megaseconds, to X-ray variable Active Galactic Nuclei (AGN) research. This would enable reverberation studies, already a commonplace feature of AGN, to proceed to the next level and follow the behaviour of the powerful dynamic corona. Such a dedicated legacy programme can only be carried out with XMM-Newton.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-11-21T17:24:24.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "x-ray reverberation",
      "x-ray variable active galactic nuclei",
      "luminous accreting black holes work",
      "powerful dynamic corona",
      "commonplace feature"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 5,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}