{
  "id": "astro-ph/0612429",
  "version": "v1",
  "published": "2006-12-15T13:14:14.000Z",
  "updated": "2006-12-15T13:14:14.000Z",
  "title": "The Spectral Energy Distributions of AGN with Double-Peaked Balmer Lines",
  "authors": [
    "I. Strateva",
    "W. N. Brandt",
    "M. Eracleous",
    "G. Garmire",
    "S. Komossa"
  ],
  "comment": "Conference proceedings to appear in \"The Central Engine of Active Galactic Nuclei\", ed. L. C. Ho and J.-M. Wang (San Francisco: ASP)",
  "categories": [
    "astro-ph"
  ],
  "abstract": "We summarize the optical, UV, and X-ray properties of double-peaked emitters -- AGN with double-peaked Balmer emission lines believed to originate in the AGN accretion disk. We focus on the X-ray spectroscopic results obtained from a new sample of the 16 broadest Balmer line AGN observed with Chandra and Swift.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2006-12-15T13:14:14.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "spectral energy distributions",
      "double-peaked balmer lines",
      "balmer emission lines",
      "broadest balmer line agn",
      "agn accretion disk"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 734656
    }
  }
}