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The systematic search for z≳5 active galactic nuclei in the Chandra Deep Field South

Weigel, Anna K. ; Schawinski, Kevin ; Treister, Ezequiel ; Urry, C. Megan ; Koss, Michael ; Trakhtenbrot, Benny

In: Monthly Notices of the Royal Astronomical Society, 2015, vol. 448, no. 4, p. 3167-3195

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    Titel
    • The systematic search for z≳5 active galactic nuclei in the Chandra Deep Field South
    Autor
    • Weigel, Anna K.. Institute for Astronomy, Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich, Switzerland
    • Schawinski, Kevin. Institute for Astronomy, Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich, Switzerland
    • Treister, Ezequiel. Universidad de Concepción, Departamento de Astronomía, Casilla 160-C, Concepción, Chile
    • Urry, C. Megan. Physics Department and Yale Center for Astronomy and Astrophysics, Yale University, New Haven, CT 06511, USA
    • Koss, Michael. Institute for Astronomy, Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich, Switzerland
    • Trakhtenbrot, Benny. Institute for Astronomy, Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich, Switzerland
    Dokumententyp
    • Postprint
    Sprache
    • Englisch
    Veröffentlicht in
    • Monthly Notices of the Royal Astronomical Society, 2015, vol. 448, no. 4, p. 3167-3195. Oxford University Press
    Andere elektronische Ausgabe
    OAI-PMH-ID
    • oai:doc.rero.ch:295798
    Summary
    We investigate early black hole (BH) growth through the methodical search for z≳5 active galactic nuclei (AGN) in the Chandra Deep Field South. We base our search on the Chandra 4-Ms data with flux limits of 9.1×10−18 (soft, 0.5-2 keV) and 5.5×10−17 erg s−1 cm−2 (hard, 2-8 keV). At z∼5, this corresponds to luminosities as low as ∼1042 (∼1043) erg s−1 in the soft (hard) band and should allow us to detect Compton-thin AGN with MBH>107 M⊙ and Eddington ratios >0.1. Our field (0.03 deg2) contains over 600z∼5 Lyman Break Galaxies. Based on lower redshift relations, we would expect ∼20 of them to host AGN. After combining the Chandra data with Great Observatories Origins Deep Survey (GOODS)/Advanced Camera for Surveys (ACS), CANDELS/Wide Field Camera 3 and Spitzer/Infrared Array Camera data, the sample consists of 58 high-redshift candidates. We run a photometric redshift code, stack the GOODS/ACS data, apply colour criteria and the Lyman Break Technique and use the X-ray Hardness Ratio. We combine our tests and using additional data find that all sources are most likely at low redshift. We also find five X-ray sources without a counterpart in the optical or infrared which might be spurious detections. We conclude that our field does not contain any convincing z≳5 AGN. Explanations for this result include a low BH occupation fraction, a low AGN fraction, short, super-Eddington growth modes, BH growth through BH-BH mergers or in optically faint galaxies. By searching for z≳5 AGN, we are setting the foundation for constraining early BH growth and seed formation scenarios