A disc wind model for blueshifts in quasar broad emission lines

Accepted/In Press date: 18 September 2023

e-pub ahead of print date: 28 September 2023

Published date: 1 December 2023

Additional Information: Funding Information: We thank the referee for reviewing our paper and their constructive comments. We would like to thank Andrew Sellek, Stuart Sim, Nico Scepi, and Teo Muñoz-Darias for helpful discussions. JM acknowledges support from a Royal Society University Research Fellowship and, previously, the Herchel Smith fund. ALR acknowledges support from a UKRI Future Leaders Fellowship (grant MR/T020989/1). MJT acknowledges support from a FONDECYT postdoctoral fellowship (3220516). This work was performed using resources provided by the Cambridge Service for Data Driven Discovery (CSD3) operated by the University of Cambridge Research Computing Service ( www.csd3.cam.ac.uk ), provided by Dell EMC and Intel using Tier-2 funding from the Engineering and Physical Sciences Research Council (capital grant EP/T022159/1), and DiRAC funding from the Science and Technology Facilities Council ( www.dirac.ac.uk ). We gratefully acknowledge the use of the following software packages: OpenMPI (Gabriel et al. ), matplotlib (Hunter ), and astropy (Astropy Collaboration , ). For the purpose of open access, the authors have applied a Creative Commons Attribution (CC BY) licence to any Author Accepted Manuscript version arising from this submission. Funding Information: Funding for the SDSS IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High Performance Computing at the University of Utah. The SDSS website is www.sdss4.org . SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics| Harvard & Smithsonian, the Chilean Participation Group, the French Participation Group, Instituto de Astrofísica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut für Astrophysik Potsdam (AIP), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Max-Planck-Institut für Astrophysik (MPA Garching), Max-Planck-Institut für Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State University, New York University, University of Notre Dame, Observatário Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autónoma de México, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University. Publisher Copyright: © 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Keywords: astro-ph.GA, astro-ph.HE, quasars: emission lines, quasars: general, line: formation, galaxies: active, radiative transfer, accretion, accretion discs

Local EPrints ID: 483051

URI: http://eprints.soton.ac.uk/id/eprint/483051

DOI: doi:10.1093/mnras/stad2895

ISSN: 1365-2966

PURE UUID: 2248e9d2-f43d-4335-827d-dc9a38727854

ORCID for Manda Banerji: orcid.org/0000-0002-0639-5141

Date deposited: 20 Oct 2023 16:51

Last modified: 18 Mar 2024 03:57