Mean Occupation Function of High Redshift Quasars from the Planck Cluster Catalog
arXiv:1801.06522 · doi:10.1088/1538-3873/aaab3e
Abstract
We characterise the distribution of quasars within dark matter halos using a direct measurement technique for the first time at redshifts as high as . Using the Planck Sunyaev-Zeldovich (SZ) catalogue for galaxy groups and the Sloan Digital Sky Survey (SDSS) DR12 quasar dataset, we assign host clusters/groups to the quasars and make a measurement of the mean number of quasars within dark matter halos as a function of halo mass. We find that a simple power-law fit of can be used to model the quasar fraction in dark matter halos. This suggests that the quasar fraction increases monotonically as a function of halo mass even to redshifts as high as .
Accepted for publication in PASP
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