Figure 11

Figure 11: Joint probability distributions of overdensity fields for dark halos and galaxies with dark matter overdensity smoothed over $−1 Rs = 12h Mpc$ at redshift $z = 0$ , $1$ , and $2$ . Solid lines indicate the conditional mean $¯ δi(δm )$ for each object. Dashed lines in each panel depict the theoretical prediction of conditional mean by Taruya and Suto [87]. (Figure taken from [103].)