1 INTRODUCTION

2 THE DATA

3 CLUSTERING ANALYSIS
3.1 The Angular Correlation Function
3.2 Relation to spatial quantities

4 CONNECTION WITH PHYSICAL PROPERTIES: THE HALO BIAS APPROACH

5 THE REDSHIFT EVOLUTION OF CLUSTERING OF FIR GALAXIES
5.1 Dealing with redshift dependence
5.2 Results and comparisons with other works

6 CONCLUSIONS