A simple model to link the properties of quasars to the properties of dark matter halos out to high redshift
arXiv:0901.4104 · doi:10.1111/j.1365-2966.2009.14429.x
Abstract
We present a simple model of how quasars occupy dark matter halos from z=0 to z=5 using the observed mBH-sigma relation and quasar luminosity functions. This provides a way for observers to statistically infer host halo masses for quasar observations using luminosity and redshift alone. Our model is deliberately simple and sidesteps any need to explicitly describe the physics. In spite of its simplicity, the model reproduces many key observations and has predictive power: 1) model quasars have the correct luminosity function (by construction) and spatial clustering (by consequence); 2) we predict high redshift quasars of a given luminosity live in less massive dark matter halos than the same luminosity quasars at low redshifts; 3) we predict a factor of ~5 more 10^8.5Msun black holes at z~2 than is currently observed; 4) we predict a factor of ~20 evolution in the amplitude of the mBH-Mhalo relation between z=5 and the present day; 5) we expect luminosity dependent quasar lifetimes of between tQ~10^(7-8)yr, but which may become as short as 10^(5-6)yr for quasars brighter than L*; 6) while little luminosity dependent clustering evolution is expected at z<1, increasingly strong evolution is predicted for L>L* quasars at higher redshifts. These last two results arise from the narrowing distribution of halo masses that quasars occupy as the Universe ages. We also deconstruct both "downsizing" and "upsizing" trends predicted by the model at different redshifts and space densities. Importantly, this work illustrates how current observations cannot distinguish between more complicated physically motivated quasar models and our simple phenomenological approach. It highlights the opportunities such methodologies provide.
13 pages, 10 figures, accepted for publication in MNRAS. NOTE: the millennium simulation mock quasar catalogues generated for this paper are available for public download at http://web.me.com/darrencroton/Homepage/Quasar.html (16 mocks covering z=5 to z=0)
References in corpus (17)
- A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity
- A unified model for AGN feedback in cosmological simulations of structure formation
- Direct cosmological simulations of the growth of black holes and galaxies
- A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: II. Formation of Red Ellipticals
- Clustering of High Redshift () Quasars from the Sloan Digital Sky Survey
- A synthesis model for AGN evolution: supermassive black holes growth and feedback modes
- The 2dF-SDSS LRG and QSO Survey: QSO clustering and the L-z degeneracy
- Clustering Analyses of 300,000 Photometrically Classified Quasars--I. Luminosity and Redshift Evolution in Quasar Bias
- Black Hole Growth in Hierarchical Galaxy Formation
- Luminosity and redshift dependent quasar clustering
- Constructing Merger Trees that Mimic N-Body Simulations
- Quasar Clustering at $25\kpch$ from a Complete Sample of Binaries
- The Co-Formation of Spheroids and Quasars Traced in their Clustering
- The Luminosity Function of high-redshift QSOs - A combined analysis of GOODS and SDSS
- Constraints on the correlation between QSO luminosity and host halo mass from high-redshift quasar clustering
- Quasars: What turns them off?
- The effect of stellar feedback and quasar winds on the AGN population
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- The clustering of intermediate redshift quasars as measured by the Baryon Oscillation Spectroscopic Survey
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- Reproducing the Stellar Mass/Halo Mass Relation in Simulated LCDM Galaxies: Theory vs Observational Estimates
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- The Halo Occupation Distribution of X-ray-Bright Active Galactic Nuclei: A Comparison with Luminous Quasars
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