1. INTRODUCTION

2. DATA
2.1. Calibrations of Stellar Mass and SFR

3. GALAXY SAMPLES

4. ANALYSIS METHOD
4.1. The two-point correlation function
4.2. DEEP2 Masks and 1/Vmax

5. GALAXY CLUSTERING RESULTS
5.1. Clustering Dependence on Stellar Mass
5.2. Clustering Dependence on Star Formation Rate
5.3. Clustering Dependence on Specific Star Formation Rate

6. DISCUSSION
6.1. Large-scale Clustering Behavior
6.2. Clustering Amplitude and the SFR M* Relationship
6.3. Comparison with Environment Studies
6.4. Small-scale Clustering Behavior

7. CONCLUSIONS