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It is pointed out that most schemes for determining the mass function of virialized objects from the statistics of the initial density perturbation field suffer from the cloud-in-cloud problem of miscounting the number of low-mass clumps, many of which would have been subsumed into larger objects. The paper proposes a solution based on the theory of the excursion sets of F(r, Rf), the four-dimensional initial density perturbation field smoothed with a continuous hierarchy of filters of radii R sub f.
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Bond et al. (Tue,) studied this question.
synapsesocial.com/papers/69d9fdbb5e5bcb4e3b8384d3 — DOI: https://doi.org/10.1086/170520
J. Richard Bond
University of Toronto
Shaun Cole
Northern Illinois University
G. Efstathiou
Canadian Institute for Advanced Research
The Astrophysical Journal
University of California, Berkeley
University of Oxford
Canadian Institute for Theoretical Astrophysics
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