Papers

Bolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in the XMM-COSMOS survey

  1. E. Lusso1,2,*,
  2. A. Comastri2,
  3. B. D. Simmons3,4,
  4. M. Mignoli2,
  5. G. Zamorani2,
  6. C. Vignali2,5,
  7. M. Brusa6,
  8. F. Shankar7,
  9. D. Lutz6,
  10. J. R. Trump8,
  11. R. Maiolino9,10,
  12. R. Gilli2,
  13. M. Bolzonella2,
  14. S. Puccetti11,
  15. M. Salvato6,12,
  16. C. D. Impey13,
  17. F. Civano14,
  18. M. Elvis14,
  19. V. Mainieri15,
  20. J. D. Silverman16,
  21. A. M. Koekemoer17,
  22. A. Bongiorno9,
  23. A. Merloni6,12,
  24. S. Berta6,
  25. E. Le Floc'h18,
  26. B. Magnelli6,
  27. F. Pozzi5,
  28. L. Riguccini18

Article first published online: 2 AUG 2012

DOI: 10.1111/j.1365-2966.2012.21513.x

Issue

Monthly Notices of the Royal Astronomical Society

Monthly Notices of the Royal Astronomical Society

Volume 425, Issue 1, pages 623–640, 1 September 2012

Additional Information

How to Cite

Lusso, E., Comastri, A., Simmons, B. D., Mignoli, M., Zamorani, G., Vignali, C., Brusa, M., Shankar, F., Lutz, D., Trump, J. R., Maiolino, R., Gilli, R., Bolzonella, M., Puccetti, S., Salvato, M., Impey, C. D., Civano, F., Elvis, M., Mainieri, V., Silverman, J. D., Koekemoer, A. M., Bongiorno, A., Merloni, A., Berta, S., Le Floc'h, E., Magnelli, B., Pozzi, F. and Riguccini, L. (2012), Bolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in the XMM-COSMOS survey. Monthly Notices of the Royal Astronomical Society, 425: 623–640. doi: 10.1111/j.1365-2966.2012.21513.x

Author Information

  1. 1

    Max Planck Institut für Astronomie, Heidelberg, Germany

  2. 2

    INAF–Osservatorio Astronomico di Bologna, Bologna, Italy

  3. 3

    Astronomy Department, Yale University, New Haven, CT, USA

  4. 4

    Yale Center For Astronomy & Astrophysics, Physics Department, Yale University, New Haven, CT, USA

  5. 5

    Dipartimento di Astronomia, Università di Bologna, Bologna, Italy

  6. 6

    Max Planck Institut für Extraterrestische Physik, Garching bei München, Germany

  7. 7

    GEPI, Observatoire de Paris, CNRS, Meudon, France

  8. 8

    University of California Observatories/Lick Observatory, University of California, Santa Cruz, CA, USA

  9. 9

    INAF – Osservatorio Astronomico di Roma, Monte Porzio Catone (RM), Italy

  10. 10

    Cavendish Laboratory, University of Cambridge, Cambridge

  11. 11

    ASI Science Data Center, Frascati, Italy

  12. 12

    Max Planck Institut für Plasma Physik and Excellence Cluster, Garching, Germany

  13. 13

    Steward Observatory, University of Arizona, Tucson, AZ, USA

  14. 14

    Harvard–Smithsonian Center for Astrophysics, Cambridge, MA, USA

  15. 15

    ESO, Garching bei München, Germany

  16. 16

    Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, Kashiwashi, Chiba, Japan

  17. 17

    Space Telescope Science Institute, Baltimore, MD, USA

  18. 18

    Laboratoire AIM, CEA/DSM-CNRS-Université Paris Diderot, Gif-sur-Yvette Cedex, France

*E-mail: lusso@mpia.de

Publication History

  1. Issue published online: 20 AUG 2012
  2. Article first published online: 2 AUG 2012
  3. Manuscript Accepted: 12 JUN 2012
  4. Manuscript Received: 6 JUN 2012

Funded by

  • ASI-INAF. Grant Numbers: I/009/10/0, I/088/06, ASI/COFIS/WP3110, I/026/07/0
  • Bundesministerium für Wirtshaft und Techologie/Deutsches Zentrum für Luft und Raumfahrt
  • Max Planck Society
  • German Deutsche Forschungsgemeinschaft
  • DFG Leibniz. Grant Number: FKZ HA 1850/28-1
  • Marie Curie

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