%0 Journal Article
%T The Quasar-LBG Two-point Angular Cross-correlation Function at z ~ 4 in the COSMOS Field
%A H. Ikeda
%A T. Nagao
%A Y. Taniguchi
%A K. Matsuoka
%A M. Kajisawa
%A M. Akiyama
%A T. Miyaji
%A N. Kashikawa
%A T. Morokuma
%A Y. Shioya
%A M. Enoki
%A P. Capak
%A A. M. Koekemoer
%A D. Masters
%A M. Salvato
%A D. B. Sanders
%A E. Schinnerer
%A N. Z. Scoville
%J Physics
%D 2015
%I arXiv
%R 10.1088/0004-637X/809/2/138
%X In order to investigate the origin of quasars, we estimate the bias factor for low-luminosity quasars at high redshift for the first time. In this study, we use the two-point angular cross-correlation function (CCF) for both low-luminosity quasars at $-24<M_{\rm 1450}<-22$ and Lyman-break galaxies (LBGs). Our sample consists of both 25 low-luminosity quasars (16 objects are spectroscopically confirmed low-luminosity quasars) in the redshift range $3.1<z<4.5$ and 835 color-selected LBGs with $z^{\prime}_{\rm LBG}<25.0$ at $z\sim4$ in the COSMOS field. We have made our analysis for the following two quasar samples; (1) the spectroscopic sample (the 16 quasars confirmed by spectroscopy), and (2) the total sample (the 25 quasars including 9 quasars with photometric redshifts). The bias factor for low-luminosity quasars at $z\sim4$ is derived by utilizing the quasar-LBG CCF and the LBG auto-correlation function. We then obtain the $86\%$ upper limits of the bias factors for low-luminosity quasars, that are 5.63 and 10.50 for the total and the spectroscopic samples, respectively. These bias factors correspond to the typical dark matter halo masses, log $(M_{\rm DM}/(h^{-1}M_{\odot}))=$$12.7$ and $13.5$, respectively. This result is not inconsistent with the predicted bias for quasars which is estimated by the major merger models.
%U http://arxiv.org/abs/1507.05292v2