The Chandra Deep Proto-cluster Field: Black-Hole Growth and Feedback in Dense Environments

Details The Chandra Deep Proto-cluster Field: Black-Hole Growth and Feedback in Dense Environments The Chandra Deep Proto-cluster Field: Black-Hole Growth and Feedback in Dense Environments

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cxo..prop.2248a&link_type=abstract

Chandra Proposal ID #08900745

Computer Science

Chandra Proposal Id #08900745

Scientific paper

Deep X-ray surveys have revolutionized our understanding of the growth of black holes (SMBH). But these surveys only sample low-density regions at high-z due to their limited solid angle. There is no comparably sensitive X-ray census of AGN in high-density regions at high-z. Such environments evolve into the most massive clusters at z=0, regions which exhibit remarkable trends in galaxy properties - which may reflect early interactions between SMBHs and their host galaxies. A survey of a proto-cluster at high-z would provide a unique view of the interplay of the growth of galaxies and their SMBHs. Here we propose a 400ks survey of the best-studied proto-cluster at high-z, to enable the first definitive study of the growth of SMBHs and their host galaxies in a dense, young, environment.

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