{ "id": "0908.3908", "version": "v1", "published": "2009-08-26T21:19:46.000Z", "updated": "2009-08-26T21:19:46.000Z", "title": "Binary Quasars at High Redshift II: Sub-Mpc Clustering at z ~ 3-4", "authors": [ "Yue Shen", "Joseph F. Hennawi", "Francesco Shankar", "Adam D. Myers", "Michael A. Strauss", "S. G. Djorgovski", "Xiaohui Fan", "Carlo Giocoli", "Ashish Mahabal", "Donald P. Schneider", "David H. Weinberg" ], "comment": "Submitted to ApJ", "categories": [ "astro-ph.CO", "astro-ph.GA" ], "abstract": "We present measurements of the small-scale (0.1<~ r <~ 1 Mpc/h) quasar two-point correlation function at z>2.9, for a flux-limited (i<21) sample of 15 binary quasars compiled by Hennawi et al. (2009). The amplitude of the small-scale clustering increases from z ~ 3 to z ~ 4. The small-scale clustering amplitude is comparable to or lower than power-law extrapolations (with slope gamma=2) from the large-scale correlation function of the i<20.2 quasar sample from the Sloan Digital Sky Survey. Using simple prescriptions relating quasars to dark matter halos, we model the observed small-scale clustering with halo occupation models. Reproducing the large-scale clustering amplitude requires that the active fraction of the black holes in the central galaxies of halos is near unity, but the level of small-scale clustering favors an active fraction of black holes in satellite galaxies 0.1 <~ f_s <~ 0.5 at z >~ 3.", "revisions": [ { "version": "v1", "updated": "2009-08-26T21:19:46.000Z" } ], "analyses": { "keywords": [ "high redshift", "binary quasars", "sub-mpc clustering" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/719/2/1693", "journal": "The Astrophysical Journal", "year": 2010, "month": "Aug", "volume": 719, "number": 2, "pages": 1693 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 829588, "adsabs": "2010ApJ...719.1693S" } } }