The Active Galaxy Population in a Supercluster at z = 0.7

Details The Active Galaxy Population in a Supercluster at z = 0.7 The Active Galaxy Population in a Supercluster at z = 0.7

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2450l&link_type=abstract

Chandra Proposal ID #09800484

Physics

Chandra Proposal Id #09800484

Scientific paper

We propose to use Chandra and the VLA to map the active galaxy population in a supercluster at z = 0.7. The structure contains seven massive clusters and covers a 11 Mpc x 22 Mpc region. Combined with our extensive supporting data, the Chandra and VLA observations will allow us to measure the properties of X-ray and radio sources over a wide range of local densities, study AGN/starburst host galaxies to determine what causes gas-fueling events, and quantify the effect of large scale structure on the nuclear activity and gas content of galaxies. The proposed observations will be used to constrain how large-scale processes influence galaxy-scale events and are a natural continuation of our approved Cycle 7 & 8 programs to study superclusters and dynamically-active systems at high redshift.

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