Halo occupation numbers and galaxy bias
J. A. PeacockInstitute for Astronomy University of Edinburgh Royal Observatory, Blackford Hill Edinburgh EH9 3HJR. C. SmithInstitute for Astronomy University of Edinburgh Royal Observatory, Blackford Hill Edinburgh EH9 3HJ
2000en
ABI
Abstract
The large-scale structure in the distribution of galaxies has long been assumed to arise from primordial inhomogeneities in the cosmological mass distribution. The quantitative study of the evolution of these inhomogeneities is
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Cited by 20 references