Galaxy correlation functions in redshift space from large N-body simulations

Statistics – Computation

Scientific paper

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Computational Astrophysics, Galactic Clusters, Many Body Problem, Red Shift, Astronomical Models, Dark Matter, Gravitational Effects

Scientific paper

Galaxy-galaxy correlation functions are computed in redshift space with
data from a set of large cold dark matter N-body simulations. When the
velocity dispersion is computed by direct pair counts, the best match is
for a bias factor b = 1.4.

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