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Binary Quasars at High Redshift. II. Sub-Mpc Clustering at z ~ 3-4

Shen, Yue and Hennawi, Joseph F. and Shankar, Francesco and Myers, Adam D. and Strauss, Michael A. and Djorgovski, S. G. and Fan, Xiaohui and Giocoli, Carlo and Mahabal, Ashish and Schneider, Donald P. and Weinberg, David H. (2010) Binary Quasars at High Redshift. II. Sub-Mpc Clustering at z ~ 3-4. Astrophysical Journal, 719 (2). pp. 1693-1698. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20100903-105120337

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Abstract

We present measurements of the small-scale (0.1 ≲ r ≲ 1 h^(-1) Mpc) 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. 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 (assuming a fixed slope γ = 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. We found that the level of small-scale clustering favors an active fraction of black holes in (M ≳ 10^(13) h^(–1) M_☉) satellite halos f_s ≳ 0.1 at z ≳ 3.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/719/2/1693DOIArticle
http://iopscience.iop.org/0004-637X/719/2/1693/PublisherArticle
ORCID:
AuthorORCID
Shen, Yue0000-0003-1659-7035
Hennawi, Joseph F.0000-0002-7054-4332
Strauss, Michael A.0000-0002-0106-7755
Djorgovski, S. G.0000-0002-0603-3087
Fan, Xiaohui0000-0003-3310-0131
Mahabal, Ashish0000-0003-2242-0244
Additional Information:© 2010 American Astronomical Society. Received 2009 August 25; accepted 2010 March 19; published 2010 August 3. We thank the anonymous referee for useful comments and Silvia Bonoli, Charlie Conroy, Phil Hopkins, and Linhua Jiang for helpful discussions. This work was partially supported by NSF grants AST-0707266 (Y.S. and M.A.S.) and AST-0607634 (D.P.S.). Y.S. acknowledges partial support from a Clay Postdoctoral Fellowship through the Smithsonian Astrophysical Observatory (SAO). F.S. acknowledges partial support from NASA 17 Although we do not have the adequate simulation data set, we compared the Giocoli et al. subhalo mass function with the alternative prescription in Tinker & Conroy (2009). We found that the difference in the two subhalo mass functions has negligible effects on our conclusions. grant NNG05GH77G and from the Alexander von Humboldt Foundation. S.G.D. and A.M. acknowledge partial support from NSF grant AST-0407448 and the Ajax Foundation.
Funders:
Funding AgencyGrant Number
NSFAST-0707266
NSFAST-0607634
Smithsonian Astrophysical ObservatoryUNSPECIFIED
NASANNG05GH77G
Alexander von Humboldt FoundationUNSPECIFIED
NSFAST-0407448
Ajax FoundationUNSPECIFIED
Subject Keywords:black hole physics; cosmology: observations; galaxies: active; large-scale structure of universe; quasars: general; surveys
Issue or Number:2
Classification Code:PACS: 98.54.Aj; 95.85.Kr; 95.35.+d; 98.62.Py; 98.62.Js; 98.65.Dx
Record Number:CaltechAUTHORS:20100903-105120337
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20100903-105120337
Official Citation:Yue Shen et al 2010 ApJ 719 1693 doi: 10.1088/0004-637X/719/2/1693
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:19779
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:08 Sep 2010 14:37
Last Modified:09 Mar 2020 13:19

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