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.Comment: 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
