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Host galaxies and large-scale structures of active galactic nuclei

Published online by Cambridge University Press:  27 October 2016

Ryan C. Hickox ,
Stephanie M. LaMassa ,
John D. Silverman  and
Alexander Kolodzig
Ryan C. Hickox
Affiliation:
Department of Physics and Astronomy, Dartmouth College, 6127 Wilder Laboratory, Hanover, NH 03755, USA email: ryan.c.hickox@dartmouth.edu
Stephanie M. LaMassa
Affiliation:
NASA Goddard Space Flight Center, Code 662, Greenbelt, MD 20771, USA
John D. Silverman
Affiliation:
Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan
Alexander Kolodzig
Affiliation:
Kavli Institute for Astronomy and Astrophysics (KIAA), Peking University, 100871 Beijing, China
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Abstract

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Our understanding of the cosmic evolution of supermassive black holes (SMBHs) has been revolutionized by the advent of large multiwavelength extragalactic surveys, which have enabled detailed statistical studies of the host galaxies and large-scale structures of active galactic nuclei (AGN). We give an overview of some recent results on SMBH evolution, including the connection between AGN activity and star formation in galaxies, the role of galaxy mergers in fueling AGN activity, the nature of luminous obscured AGN, and the connection between AGN and their host dark matter halos. We conclude by looking to the future of large-scale extragalactic X-ray and spectroscopic surveys.

Keywords

(galaxies:) quasars: generalgalaxies: SeyfertsurveysX-rays: galaxies(cosmology:) large-scale structure of universe
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 113 - 123
Copyright
Copyright © International Astronomical Union 2016 

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