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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. 11.

Upper panels: Two‐point correlation functions for dark matter and DM cores at redshifts ﹩z=0﹩, 1, and 2. Middle panels: Two‐point correlation functions for dark matter, galaxies, and dark halos. Lower panels: Profiles of biasing parameter ﹩b_{\xi }( r) ﹩ for dark halos, DM cores, and galaxies at ﹩z=0﹩, 1, and 2; we also plot the parameter ﹩b_{\mathrm{var}\,}﹩ on the smoothing scales ﹩R_{s}=4﹩, 8, and 12 h−1 Mpc at ﹩r=R_{s}﹩ for each kind of object by different symbols.

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