{
  "id": "astro-ph/0306411",
  "version": "v1",
  "published": "2003-06-20T10:25:56.000Z",
  "updated": "2003-06-20T10:25:56.000Z",
  "title": "Highlights from XMM-Newton",
  "authors": [
    "X. Barcons",
    "I. Negueruela"
  ],
  "comment": "21 pages, inivited paper to appear in the \"Boletin de la SEA\", July 2003 issue (electronic release at http://sea.am.ub.es)",
  "categories": [
    "astro-ph"
  ],
  "abstract": "The launch of the Chandra (NASA) and XMM-Newton (ESA) X-ray observatories in 1999 has revolutionized our view of the Universe, by providing astrophysical information about many classes of sources with unprecedent detail. The high throughput of XMM-Newton makes it the ideal instrument to provide low to moderate resolution spectroscopy of faint and extended sources. After 3 years of operations, XMM-Newton has observed many types of astronomical sources and delivered very interesting results in many areas. In this review, we highlight a few points where the contribution of XMM-Newton has significantly furthered our knowledge of the energetic Universe.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2003-06-20T10:25:56.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "xmm-newton",
      "moderate resolution spectroscopy",
      "energetic universe",
      "x-ray observatories",
      "ideal instrument"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 21,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 621595,
      "adsabs": "2003astro.ph..6411B"
    }
  }
}