Proto-Clusters Around High-Redshift Radio Galaxies

Details Proto-Clusters Around High-Redshift Radio Galaxies Proto-Clusters Around High-Redshift Radio Galaxies

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop...79f&link_type=abstract

Spitzer Proposal ID #79

Physics

Scientific paper

High-redshift radio galaxies (HzRGs) provide our most robust examples of massive galaxies at early cosmic epoch. In biased galaxy formation models, we therefore expect associated galaxy overdensities around HzRGs. In this program we undertake deep IRAC, MIPS, and IRS observations of two distant radio galaxies, each of which once held the record for most distant galaxy known. These fields have also been subjected to deep optical (ground-based and Hubble) and sub-mm observations. We will attempt to identify possible galaxy proto-clusters surrounding these high-redshift AGN.

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