Mathematics – Probability
Scientific paper
Jan 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21710605h&link_type=abstract
American Astronomical Society, AAS Meeting #217, #106.05; Bulletin of the American Astronomical Society, Vol. 43, 2011
Mathematics
Probability
Scientific paper
The growth of massive galaxies and their central supermassive black holes is linked to the their surrounding dark matter halos, whose masses can be inferred from measurements of spatial clustering. I will present a a novel technique for deriving real-space clustering using full photometric-redshift probability distributions, and discuss a recent study using this technique to measure clustering of dust-obscured (Type 2) and unobscured (Type 1) luminous quasars. I will present a similar measurement of the clustering of submillimeter galaxies, and will place the results in context of current models for the co-evolution of quasars and rapid starbursts. Finally I will briefly point toward future observational opportunities with Herschel and the proposed Wide Field X-ray Telescope mission. RCH is funded by an STFC Postdoctoral Fellowship.
Bootes Survey Collaboration
Hickox Ryan C.
Myers Adam D.
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