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Article Contents

ABSTRACT

1.HISTORICAL BACKGROUND

2.THE TWO-POINT CORRELATION FUNCTION

3.ANGULAR CLUSTERING

4.REAL AND REDSHIFT SPACE CLUSTERING

5.GALAXY BIAS

6.THE DEPENDENCE OF CLUSTERING ON GALAXY PROPERTIES

6.1.Luminosity Dependence

6.2.Color and Spectral Type Dependence

6.3.Redshift Space Distortions

7.THE EVOLUTION OF GALAXY CLUSTERING

8.HALO MODEL INTERPRETATION of (r)

8.1.Estimating the Mean Halo Mass from the Bias

8.2.Halo Occupation Distribution Modeling

8.3.Interpreting the Luminosity and Color Dependence of Galaxy Clustering

8.4.Interpreting the Evolution of Galaxy Clustering

9.VOIDS AND FILAMENTS

9.1.Higher-order Clustering Measurements

9.2.Voids

9.2.1.Void and Void Galaxy Properties

9.2.2.Void Probability Function

9.3.Filaments

10.SUMMARY AND FUTURE

REFERENCES