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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. 8.

Relation between environmental temperature and the ratios of dark matter overdensity with that of galaxies with ﹩z_{f}> 1.7﹩ (left panel) and ﹩z_{f}< 1.7﹩ (right panel) in the high‐density regions (﹩\delta _{m}> 5﹩). Each point corresponds to the randomly selected point in the simulation box. Smoothing scale is set to ﹩R_{s}=4\,h^{-1}﹩ Mpc.

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