Fig. 2

The mean bias , as a function of
distance x, at redshift z = 0 for halos defined by
the nonlinear density threshold δ∗ = 200. We show our
results from Eq. (30) for the five
mass bins
1013 < M < 3 × 1013 h-1M⊙,
3 × 1013 < M < 1014 h-1M⊙,
1014 < M < 3 × 1014 h-1M⊙,
3 × 1014 < M < 1015 h-1M⊙,
and
1015 < M < 3 × 1015 h-1M⊙,
from bottom to top.
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