{
  "id": "astro-ph/0106203",
  "version": "v1",
  "published": "2001-06-12T13:55:44.000Z",
  "updated": "2001-06-12T13:55:44.000Z",
  "title": "CHANDRA observation of the narrow-line Seyfert 1 galaxy IRAS 13224-3809",
  "authors": [
    "F. Pfefferkorn",
    "Th. Boller",
    "V. Burwitz",
    "P. Predehl"
  ],
  "comment": "5 pages, 10 figures, 1 table, proceedings paper for the \"MAXI workshop on AGN variability\" held in Nikko, Japan (March 10-11, 2001), also available at http://www.xray.mpe.mpg.de/~pfefferk/research/proceedings.html",
  "categories": [
    "astro-ph"
  ],
  "abstract": "The narrow-line Seyfert 1 galaxy (NLS1) IRAS 13224-3809 has been observed with the CHANDRA High Resolution Camera (HRC-I) for 12 ksec on February, 2, 2000. The source was proposed for CHANDRA observations to precisely determine the X-ray centroid position and to investigate the timing properties of the most X-ray variable Seyfert galaxy. The position derived from CHANDRA confirms that the X-ray emission is associated with IRAS 13224-3809. The CHANDRA HRC-I light curve shows indications for a possible presence of a quasi-periodic oscillation. The strongest signal is found at 2500 sec. Accretion disk instabilities may provide a plausible explanation for the quasi-periodic oscillations.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2001-06-12T13:55:44.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "chandra observation",
      "narrow-line seyfert",
      "galaxy iras",
      "chandra high resolution camera",
      "quasi-periodic oscillation"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 5,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 575337,
      "adsabs": "2001astro.ph..6203P"
    }
  }
}