Redshift surveys of galaxies definitely serve as the central database for observational cosmology. In addition to the existing shallower surveys (), clustering in the Universe in the range has been partially revealed by, for instance, the Lyman-break galaxies and X-ray selected AGNs. In particular, the 2dF and SDSS QSO redshift surveys promise to extend the observable scale of the Universe by an order of magnitude, up to a few Gpc. A proper interpretation of such redshift surveys in terms of the clustering evolution, however, requires an understanding of many cosmological effects which can be neglected for and thus have not been considered seriously so far. These cosmological contaminations include linear redshift-space (velocity) distortion, nonlinear redshift-space (velocity) distortion, cosmological redshift-space (geometrical) distortion, and the cosmological light-cone effect.

We describe a theoretical formalism to incorporate those effects, in particular the cosmological redshift-distortion and light-cone effects, and present several specific predictions in CDM models. The details of the material presented in this section may be found in [83, 101, 100, 46, 28, 29].

5.1 Cosmological light-cone effect on the two-point correlation functions

5.2 Evaluating two-point correlation functions from N-body simulation data

5.3 Cosmological redshift-space distortion

5.4 Two-point clustering statistics on a light-cone in cosmological redshift space

5.2 Evaluating two-point correlation functions from N-body simulation data

5.3 Cosmological redshift-space distortion

5.4 Two-point clustering statistics on a light-cone in cosmological redshift space

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