1. Introduction

2. The Survey Strategy
2.1. The VIMOS Instrument
2.2. The Field Coverage: VIMOS Pointing Layout
2.3. Target Selection

3. Observations and Data Reduction
3.1. Preparation of VIMOS Observations
3.2. Data Reduction
3.3. The VIMOS LR-Blue Wiggles
3.4. Target Coordinates

4. Redshift Determination
4.1. The Success Rate

5. Discussion
5.1. Reliability of the Redshifts - Comparison with Previous Surveys
5.2. Reliability of the Redshifts - Comparison with Photometric Redshift
5.3. The Survey Completeness
5.4. Redshift Distribution and Large Scale Structure

6. Reliability of the Photometric Techniques for the Selection of Galaxies at \(1<z<3\)

7. Conclusions