1 INTRODUCTION

2 OBSERVATIONS
2.1 Survey overview
2.2 Imaging
2.3 Candidate selection
2.4 Spectroscopy
2.5 Identification of targets
2.6 LBG sample
2.7 Galaxy redshifts

3 CLUSTERING OF z≈3 LBGS
3.1 Semi-projected correlation function, wp(σ)
3.2 2D Auto-Correlation Function, ξ(σ,π)
3.3 Redshift-space correlation function, ξ(s)
3.4 Double power-law correlation function models
3.5 Estimating Ωm and the growth rate
3.6 The dark matter halos of z∼3 star-forming galaxies

4 CONCLUSIONS