Title: Measuring Luminosity Dependent Quasar Clustering

Details Title: Measuring Luminosity Dependent Quasar Clustering Title: Measuring Luminosity Dependent Quasar Clustering

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21944003k&link_type=abstract

American Astronomical Society, AAS Meeting #219, #440.03

Astronomy and Astrophysics

Astronomy

Scientific paper

Whether luminous quasars reside in dark matter halos of the same mass and accrete at different rates, or, live in haloes of different masses, and accretion is near the Eddington limit, is still an open question. Here, we present measurements of the luminosity-dependence of quasar clustering, using data from the SDSS, 2SLAQ QSO and the new SDSS-III: BOSS Quasar surveys, allowing us to span 4 magnitudes in luminosity, at a given redshift. Using a cross-correlation technique, we measure the clustering of 3100 0.5

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