{
  "id": "0902.4239",
  "version": "v1",
  "published": "2009-02-24T21:19:18.000Z",
  "updated": "2009-02-24T21:19:18.000Z",
  "title": "The Very Local Universe in X-rays",
  "authors": [
    "A. Ptak",
    "E. Feigelson",
    "Y. -H. Chu",
    "K. Kuntz",
    "A. Zezas",
    "S. Snowden",
    "D. de Martino",
    "G. Trinchieri",
    "G. Fabbiano",
    "W. Forman",
    "G. Tagliaferri",
    "R. Giacconi",
    "S. Murray",
    "S. Allen",
    "M. Bautz",
    "S. Borgani",
    "N. Brandt",
    "S. Campana",
    "M. Donahue",
    "K. Flannagan",
    "R. Gilli",
    "C. Jones",
    "N. Miller",
    "G. Pareschi",
    "P. Rosati",
    "D. Schneider",
    "P. Tozzi",
    "A. Vikhlinin"
  ],
  "comment": "8 pages, Astro2010 Science White paper. Full-resolution version available at http://wfxt.pha.jhu.edu",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "While the exceptional sensitivity of Chandra and XMM-Newton has resulted in revolutionary studies of the Galactic neighborhood in the soft (<10 keV) X-ray band, there are many open questions. We discuss these issues and how they would be addressed by very wide-area (> 100 sq. deg.) X-ray surveys.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2009-02-24T21:19:18.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "local universe",
      "exceptional sensitivity",
      "revolutionary studies",
      "galactic neighborhood"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 8,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 814123,
      "adsabs": "2009astro2010S.240P"
    }
  }
}