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The X-Ray AGN Bias Factor at Zero Redshift

Krivonos, R.~A. and Revnivtsev, M.~G.

Keywords

large-scale structure of universe, galaxies: Seyfert, X-rays: galaxies

Abstract

Using an AGN sample from the INTEGRAL all-sky survey, we show that the density fluctuations of matter in the local universe translate linearly into the density fluctuations of accreting supermassive black holes. Our results imply that hard X-ray emitting AGNs are unbiased tracers of the galaxy population in the nearby universe and SMBH activity is independent of the density of galaxies.

Information

Published
2010 as inproceedings
IAU Symposium, - page(s): 462-462
Type
experimental work
Links
pdf
ads
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Related to the research area(s):
F

Technische Universitaet Muenchen
Exzellenzcluster Universe

Boltzmannstr. 2
D-85748 Garching

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