The X-Ray AGN Bias Factor at Zero Redshift

Details The X-Ray AGN Bias Factor at Zero Redshift The X-Ray AGN Bias Factor at Zero Redshift

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..267..462k&link_type=abstract

Co-Evolution of Central Black Holes and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 267

Astronomy and Astrophysics

Astronomy

Large-Scale Structure Of Universe, Galaxies: Seyfert, X-Rays: Galaxies

Scientific paper

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.

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