A catalogue of optical to X-ray spectral energy distributions of z ≈ 2 quasars observed with Swift – I. First results

Accepted/In Press date: 16 February 2017

Published date: 1 June 2017

Additional Information: Funding Information: Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington and Yale University. Funding Information: We thank the anonymous referee for helpful feedback with regards to the X-ray modelling, and for a thorough report that improved the clarity of the manuscript as a whole. This work took advantage of the Danish Swift guaranteed time programme. We thank local Swift affiliate Daniele Malesani, and the Swift helpdesk at the University of Leicester, for their assistance in obtaining and processing the data. DL, MV and SR gratefully acknowledge support from the Danish Council for Independent Research via grant no. DFF 4002-00275. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington and Yale University. Funding Information: This work took advantage of the Danish Swift guaranteed time programme. We thank local Swift affiliate Daniele Malesani, and the Swift helpdesk at the University of Leicester, for their assistance in obtaining and processing the data. DL, MV and SR gratefully acknowledge support from the Danish Council for Independent Research via grant no. DFF 4002-00275. Publisher Copyright: © 2017 The Authors.

Keywords: Catalogues – quasars: general

Local EPrints ID: 473430

URI: http://eprints.soton.ac.uk/id/eprint/473430

DOI: doi:10.1093/mnras/stx423

ISSN: 1365-2966

PURE UUID: a71025d3-9227-4cc4-a133-122c2c00443f

ORCID for S. Raimundo: orcid.org/0000-0002-6248-398X

Date deposited: 18 Jan 2023 17:31

Last modified: 18 Mar 2024 03:58