Analytical Approximations to Galaxy Clustering

Abstract

We discuss some recent progress in constructing analytic approximations to the galaxy clustering. We show that successful models can be constructed for the clustering of both dark matter and dark matter haloes. Our understanding of galaxy clustering and galaxy biasing can be greatly enhanced by these models.

10 pages, Latex, crckapb.sty, figure included, to appear in the proceedings of Ringberg Workshop on Large-Scale Structure (ed. D. Hamilton; Kluwer Academic Publishers)

References in corpus (3)

• An analytic model for the spatial clustering of dark matter haloes
• High-Order Correlations of Peaks and Halos: a Step toward Understanding Galaxy Biasing
• The Correlation Function of Clusters of Galaxies and the Amplitude of Mass Fluctuations in the Universe