Probing Coeval Star Formation and Black Hole Growth in the Most Massive Galaxies

Details Probing Coeval Star Formation and Black Hole Growth in the Most Massive Galaxies Probing Coeval Star Formation and Black Hole Growth in the Most Massive Galaxies

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sptz.prop50379s&link_type=abstract

Spitzer Proposal ID #50379

Physics

Scientific paper

At every epoch, powerful radio galaxies are associated with the most massive galaxies known as evidenced by their tight observed-frame K-z relation which traces the bright envolope of field galaxies. We have shown (Seymour et al. 2007) that the rest-frame H-band stellar luminosities of high-z radio galaxies (HzRGs) are uniformly consistent with stellar masses of ~5x10^11 Msun across 1

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