Slicing cluster mass functions with a Bayesian razor

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

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5 pages, 2 figures, accepted to Astronomische Nachrichten

Scientific paper

10.1002/asna.201011409

We apply a Bayesian "razor" to forecast Bayes factors between different
parameterizations of the galaxy cluster mass function. To demonstrate this
approach, we calculate the minimum size N-body simulation needed for strong
evidence favoring a two-parameter mass function over one-parameter mass
functions and visa versa, as a function of the minimum cluster mass.

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