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The Illustris simulation: Evolving population of black holes across cosmic time

Sijacki, Debora and Vogelsberger, Mark and Genel, Shy and Springel, Volker and Torrey, Paul and Snyder, Gregory F. and Nelson, Dylan and Hernquist, Lars (2015) The Illustris simulation: Evolving population of black holes across cosmic time. Monthly Notices of the Royal Astronomical Society, 452 (1). pp. 575-596. ISSN 0035-8711. http://resolver.caltech.edu/CaltechAUTHORS:20141217-100812992

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Abstract

We study the properties of black holes and their host galaxies across cosmic time in the Illustris simulation. Illustris is a large-scale cosmological hydrodynamical simulation which resolves a (106.5 Mpc)^3 volume with more than 12 billion resolution elements and includes state-of-the-art physical models relevant for galaxy formation. We find that the black hole mass density for redshifts z = 0–5 and the black hole mass function at z = 0 predicted by Illustris are in very good agreement with the most recent observational constraints. We show that the bolometric and hard X-ray luminosity functions of active galactic nuclei (AGN) at z = 0 and 1 reproduce observational data very well over the full dynamic range probed. Unless the bolometric corrections are largely underestimated, this requires radiative efficiencies to be on average low, ϵ_r ≲ 0.1, noting however that in our model radiative efficiencies are degenerate with black hole feedback efficiencies. Cosmic downsizing of the AGN population is in broad agreement with the findings from X-ray surveys, but we predict a larger number density of faint AGN at high redshifts than currently inferred. We also study black hole–host galaxy scaling relations as a function of galaxy morphology, colour and specific star formation rate. We find that black holes and galaxies co-evolve at the massive end, but for low mass, blue and star-forming galaxies there is no tight relation with either their central black hole masses or the nuclear AGN activity.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1408.6842arXivDiscussion Paper
http://dx.doi.org/10.1093/mnras/stv1340 DOIArticle
http://mnras.oxfordjournals.org/content/452/1/575PublisherArticle
ORCID:
AuthorORCID
Genel, Shy0000-0002-3185-1540
Springel, Volker0000-0001-5976-4599
Torrey, Paul0000-0002-5653-0786
Additional Information:© 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2015 June 12. Received 2015 June 12. In original form 2014 August 28. First published online July 6, 2015. We would like to thank the referee for a very constructive referee report which improved this paper. DS would like to thank Martin Haehnelt, Manda Banerji, Roberto Maiolino, Matt Auger, Ranjan Vasudevan, Andy Fabian and Richard McMahon for very useful discussions. DS also would like to thank Manda Banerji for kindly providing the data compilation used in Fig. 13. Simulations were run on the Harvard Odyssey and CfA/ITC clusters, the Ranger and Stampede supercomputers at the Texas Advanced Computing Center as part of XSEDE, the Kraken supercomputer at Oak Ridge National Laboratory as part of XSEDE, the CURIE supercomputer at CEA/France as part of PRACE project RA0844 and the SuperMUC computer at the Leibniz Computing Centre, Germany, as part of project pr85je. VS acknowledges support by the DFG Research Centre SFB-881 ‘The Milky Way System’ through project A1, and by the European Research Council under ERC-StG EXAGAL-308037. SG acknowledges support provided by NASA through Hubble Fellowship grant HST-HF2-51341.001-A awarded by the STScI, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. GFS acknowledges support from the HST grants program, numbers HST-AR-12856.01-A and HST-AR-13887.004A. Support for programs #12856 and #13887 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. LH acknowledges support from NASA grant NNX12AC67G and NSF grant AST-1312095.
Group:TAPIR
Funders:
Funding AgencyGrant Number
Deutsche Forschungsgemeinschaft (DFG)SFB-881
European Research Council (ERC)EXAGAL-308037
Hubble FellowshipHST-HF2-51341.001-A
NASANAS5-26555
Hubble Space Telescope (HST)HST-AR-12856.01-A
Hubble Space Telescope (HST)HST-AR-13887.004A
Space Telescope Science InstituteUNSPECIFIED
NASANNX12AC67G
NSFAST-1312095
Subject Keywords:methods: numerical; galaxies: formation; quasars: supermassive black holes; cosmology: theory
Record Number:CaltechAUTHORS:20141217-100812992
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20141217-100812992
Official Citation:Debora Sijacki, Mark Vogelsberger, Shy Genel, Volker Springel, Paul Torrey, Gregory F. Snyder, Dylan Nelson, and Lars Hernquist The Illustris simulation: the evolving population of black holes across cosmic time MNRAS (September 01, 2015) Vol. 452 575-596 doi:10.1093/mnras/stv1340 First published online July 6, 2015
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:52950
Collection:CaltechAUTHORS
Deposited By: Joy Painter
Deposited On:17 Dec 2014 19:44
Last Modified:18 Apr 2017 18:45

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