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Nonlinear Stochastic Biasing of Galaxies and Dark Halos in Cosmological Hydrodynamic Simulations

  • Authors: Kohji Yoshikawa, Atsushi Taruya, Y. P. Jing, and Yasushi Suto

Yoshikawa et al. 2001 The Astrophysical Journal 558 520.

  • Provider: AAS Journals

Caption: Fig. 10.

Number of galaxies that reside in a dark halo (upper panels) and distributions of mass ratio between galaxies and dark halos that host them (lower panels) at redshifts ﹩z=0﹩ and 2. In lower panels, solid lines indicate the mean baryon fraction (﹩\Omega _{b}/ \Omega _{0}﹩) and dashed lines indicate the resolution limit constrained by the minimum mass of galaxies in their definition (see § 2.2).

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