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Title:
AGN and Host Galaxies in the COSMOS Survey
Authors:
Impey, Christopher D.; Trump, Jonathan R.; Gabor, Jared M.; Gabor
Affiliation:
AA(Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721), AB(University of California Observatories/Lick Observatory, University of California, Santa Cruz, CA 95064), AC(Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721), AD()
Publication:
Tracing the Ancestry of Galaxies (on the land of our ancestors), Proceedings of the International Astronomical Union, IAU Symposium, Volume 277, p. 21-25
Publication Date:
12/2011
Origin:
CUP
Abstract Copyright:
(c) 2011: Copyright © International Astronomical Union 2011
DOI:
10.1017/S1743921311022381
Bibliographic Code:
2011IAUS..277...21I

Abstract

The Cosmological Evolution Survey (COSMOS) is a unique tool for studying low level AGN activity and the co-evolution of galaxies and supermassive black holes. COSMOS involves the largest contiguous region of the sky ever imaged by HST; it includes very complete multiwavelength coverage, and the largest joint samples of galaxy and AGN redshifts in any deep survey. The result is a search for AGN with low black hole mass, low accretion rates, and levels of obscuration that can remove them from optical surveys. A complete census of intermediate mass black holes at redshifts of 1 to 3 is required to tell the story of the co-evolution of galaxies and their embedded, and episodically active, black holes.

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