Mass Functions of Supermassive Black Holes across Cosmic Time

The black hole mass function of supermassive black holes describes the evolution of the distribution of black hole mass. It is one of the primary empirical tools available for mapping the growth of supermassive black holes and for constraining theoretical models of their evolution. In this paper, we...

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Main Authors: Brandon C. Kelly, Andrea Merloni
Format: Article
Language:English
Published: Wiley 2012-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2012/970858
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author Brandon C. Kelly
Andrea Merloni
author_facet Brandon C. Kelly
Andrea Merloni
author_sort Brandon C. Kelly
collection DOAJ
description The black hole mass function of supermassive black holes describes the evolution of the distribution of black hole mass. It is one of the primary empirical tools available for mapping the growth of supermassive black holes and for constraining theoretical models of their evolution. In this paper, we discuss methods for estimating the black hole mass function, including their advantages and disadvantages. We also review the results of using these methods for estimating the mass function of both active and inactive black holes. In addition, we review current theoretical models for the growth of supermassive black holes that predict the black hole mass function. We conclude with a discussion of directions for future research which will lead to improvement in both empirical and theoretical determinations of the mass function of supermassive black holes.
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spelling doaj-art-fa4ebff99fbc41f48fbd4dd1df8718ff2025-08-20T02:22:44ZengWileyAdvances in Astronomy1687-79691687-79772012-01-01201210.1155/2012/970858970858Mass Functions of Supermassive Black Holes across Cosmic TimeBrandon C. Kelly0Andrea Merloni1High Energy Astrophysics Division, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USAMax-Planck-Institut für Extraterrestrische Physik, Giessenbachstraße 1, 85748 Garching, GermanyThe black hole mass function of supermassive black holes describes the evolution of the distribution of black hole mass. It is one of the primary empirical tools available for mapping the growth of supermassive black holes and for constraining theoretical models of their evolution. In this paper, we discuss methods for estimating the black hole mass function, including their advantages and disadvantages. We also review the results of using these methods for estimating the mass function of both active and inactive black holes. In addition, we review current theoretical models for the growth of supermassive black holes that predict the black hole mass function. We conclude with a discussion of directions for future research which will lead to improvement in both empirical and theoretical determinations of the mass function of supermassive black holes.http://dx.doi.org/10.1155/2012/970858
spellingShingle Brandon C. Kelly
Andrea Merloni
Mass Functions of Supermassive Black Holes across Cosmic Time
Advances in Astronomy
title Mass Functions of Supermassive Black Holes across Cosmic Time
title_full Mass Functions of Supermassive Black Holes across Cosmic Time
title_fullStr Mass Functions of Supermassive Black Holes across Cosmic Time
title_full_unstemmed Mass Functions of Supermassive Black Holes across Cosmic Time
title_short Mass Functions of Supermassive Black Holes across Cosmic Time
title_sort mass functions of supermassive black holes across cosmic time
url http://dx.doi.org/10.1155/2012/970858
work_keys_str_mv AT brandonckelly massfunctionsofsupermassiveblackholesacrosscosmictime
AT andreamerloni massfunctionsofsupermassiveblackholesacrosscosmictime