1 INTRODUCTION

2 IMAGING  
2.1 Target fields  
2.2 Observations  
2.3 Data Reduction  
2.4 Photometry  
2.5 Selection Criteria  
2.6 QSO Candidate Selection

3 SPECTROSCOPY  
3.1 Observations  
3.2 Data Reduction  
3.3 Object Identification  
3.4 Sky Density, Completeness & Distribution  
3.5 Velocity Offsets and Composite Spectra  
3.6 VLT AGN and QSO Observations

4 CLUSTERING  
4.1 Angular Auto-correlation Function  
4.2 Semi-Projected Correlation Function,  \(w_{p}(\sigma)\)  
4.3 Redshift-Space Correlation Function  
4.4 Estimating the LBG Infall Parameter,  \(\beta(z=3)\)  
4.5 Estimating the LBG Bias Parameter,  \(b(z=3)\)  
4.6 Further Test of the Standard Cosmology  
4.7 Clustering Evolution

5 CONCLUSIONS