Local versus Large Scale : The Active Galaxy Population in High-Redshift Clusters

Details Local versus Large Scale : The Active Galaxy Population in High-Redshift Clusters Local versus Large Scale : The Active Galaxy Population in High-Redshift Clusters

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cxo..prop.2656l&link_type=abstract

Chandra proposal ID #10800598

Computer Science

Scientific paper

We propose to use Chandra and the VLA to map the active galaxy population in two isolated, relaxed X-ray-selected clusters at z = 0.69 and 0.82, providing a vital comparison to our Cycle 7-9 programs to study high-redshift optically-selected clusters that are embedded in large scale structures or are dynamically active. Combined with our extensive photometric and spectroscopic data, the Chandra/VLA observations allow us to measure the properties of X-ray and radio sources to large clustocentric distances and study host galaxies to determine what causes gas-fueling events. Comparing with our previous studies, we can begin to disentangle the role of large-scale versus local environment in driving galaxy evolution by examining a wide range of cluster masses, dynamics, and spatial scales.

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