1. Introduction

2. Data
2.1. Object definitions and spectrum extraction
2.2. Redshift determinations
2.3. Resolving blends and final sample definition

3. Comparison to photometric redshift estimates

4. Reducing the bias in the EAZY photometric redshifts

5. Redshift outliers

6. The impact of redshift completeness

7. The impact of galaxy superpositions and blends

8. Discussion