The Halo Occupation Distribution of SDSS Quasars

Details The Halo Occupation Distribution of SDSS Quasars The Halo Occupation Distribution of SDSS Quasars

2012-03-20

arxiv.org/abs/1203.4570v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

12 pages, 4 figures, submitted to ApJ

Scientific paper

We present an estimate of the projected two-point correlation function (2PCF) of quasars in the Sloan Digital Sky Survey (SDSS) over the full range of one- and two-halo scales, 0.02-120 Mpc/h. This was achieved by combining data from SDSS DR7 on large scales and Hennawi et al. (2006; with appropriate statistical corrections) on small scales. Our combined clustering sample is the largest spectroscopic quasar clustering sample to date, containing ~48,000 quasars in the redshift range 0.4

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