1. INTRODUCTION

2. SAMPLE SELECTION
2.1. Reliability of the Photometric Redshifts
2.2. Separating Star-forming from Passive Populations

3. DERIVING STELLAR MASSES
3.1. Stellar Population Models
3.2. Mass Completeness Limits

4. THE GALAXY STELLAR MASS FUNCTION
4.1. Uncertainties due to Photometric Redshifts
4.2. Characterizing the Shape of the Mass Function
4.3. Effects of Stellar Population Models

5. DISCUSSION
5.2. Halo Mass to Stellar Mass Relation
5.3. Interpreting the Shape of the Mass Function

6. SUMMARY