Clustering Properties

Correlation Functions and Power Spectra

Figures comparing the clustering of the mass and the biased galaxy samples. In each figure the points with errorbars indicate the clustering of galaxies estimated from the APM galaxy survey (Baugh & Efstathiou 1993 and Baugh 1995 ), but scaled in amplitude to match sigma_8=0.96 as found in Maddox etal 1996

Clustering in the Mass Distributions

correlation functions and power spectra.

Clustering in the Galaxy Distributions

The correlation functions and power spectra for bias Model 1.
The correlation functions and power spectra for bias Model 2.
The correlation functions and power spectra for bias Model 3.
The correlation functions and power spectra for bias Model 4.
The correlation functions and power spectra for bias Model 5.
The correlation functions and power spectra for bias Model 6.