{
  "id": "2308.10710",
  "version": "v1",
  "published": "2023-08-18T09:59:55.000Z",
  "updated": "2023-08-18T09:59:55.000Z",
  "title": "The Accretion History of AGN: The Spectral Energy Distributions of X-ray Luminous AGN",
  "authors": [
    "Connor Auge",
    "David Sanders",
    "Ezequiel Treister",
    "C. Megan Urry",
    "Allison Kirkpatrick",
    "Nico Cappelluti",
    "Tonima Tasnim Ananna",
    "Médéric Boquien",
    "Mislav Baloković",
    "Francesca Civano",
    "Brandon Coleman",
    "Aritra Ghosh",
    "Jeyhan Kartaltepe",
    "Michael Koss",
    "Stephanie LaMassa",
    "Stefano Marchesi",
    "Alessandro Peca",
    "Meredith Powell",
    "Benny Trakhtenbrot",
    "Tracey Jane Turner"
  ],
  "comment": "24 pages, 20 figures, 4 appendix tables, Accepted to ApJ",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "Spectral energy distributions (SEDs) from X-ray to far-infrared (FIR) wavelengths are presented for a sample of 1246 X-ray luminous active galactic nuclei (AGN; $L_{0.5-10\\rm{keV}}>10^{43}$ erg s$^{-1}$), with $z_{\\rm{spec}}<1.2$, selected from Stripe 82X, COSMOS, and GOODS-N/S. The rest-frame SEDs show a wide spread ($\\sim2.5$ dex) in the relative strengths of broad continuum features at X-ray, ultraviolet (UV), mid-infrared (MIR), and FIR wavelengths. A linear correlation (log-log slope of 0.7$\\pm0.04$) is found between $L_{\\rm{MIR}}$ and $L_{\\rm{X}}$. There is significant scatter in the relation between the $L_{\\rm{UV}}$ and $L_{\\rm{X}}$ due to heavy obscuration, however the most luminous and unobscured AGN show a linear correlation (log-log slope of 0.8$\\pm0.06$) in the relation above this scatter. The relation between $L_{\\rm{FIR}}$ and $L_{\\rm{X}}$ is predominantly flat, but with decreasing dispersion at $L_{\\rm{X}}>10^{44}$ erg s$^{-1}$. The ratio between the \"galaxy subtracted\" bolometric luminosity and the intrinsic $L_{\\rm{X}}$ increases from a factor of $\\sim$$10-70$ from log $L_{\\rm{bol}}/{\\rm(erg\\; s}^{-1})=44.5-46.5$. Characteristic SED shapes have been determined by grouping AGN based on relative strengths of the UV and MIR emission. The average $L_{1\\mu\\rm{m}}$ is constant for the majority of these SED shapes, while AGN with the strongest UV and MIR emission have elevated $L_{1\\mu\\rm{m}}$, consistent with the AGN emission dominating their SEDs at optical and NIR wavelengths. A strong correlation is found between the SED shape and both the $L_{\\rm{X}}$ and $L_{\\rm{bol}}$, such that $L_{\\rm{bol}}/L_{\\rm{X}}=20.4\\pm1.8$, independent of the SED shape. This is consistent with an evolutionary scenario of increasing $L_{\\rm{bol}}$ with decreasing obscuration as the AGN blows away circumnuclear gas.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2023-08-18T09:59:55.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "spectral energy distributions",
      "x-ray luminous agn",
      "accretion history",
      "luminous active galactic nuclei",
      "agn blows away circumnuclear gas"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 24,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}