The Chandra Deep Fields and the Prevalance of Super-Massive Black Holes in the Universe

Details The Chandra Deep Fields and the Prevalance of Super-Massive Black Holes in the Universe The Chandra Deep Fields and the Prevalance of Super-Massive Black Holes in the Universe

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1340b&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

We briefly review some of the basic properties of the Chandra Deep Field (CDF) X-ray sources, explore the CDF X-ray number counts for both AGN and galaxies and how they contribute to the X-ray background, and highlight a few recent results regarding the host-galaxy morphologies of the CDF AGN using HST ACS data. We also discuss how these AGN relate to the evolution and feeding of super-massive black holes in the Universe.

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