1. INTRODUCTION

2. DATA
2.1. Galaxy Sample

3. METHOD
3.1. Correlation Function Measurement
3.2. Model Formulation

4. RESULTS
4.1. Full AGN Sample
4.2. Clustering versus Obscuration
4.3. Clustering versus Black Hole Mass

5. DISCUSSION
5.1. Environments of Local AGN
5.2. Obscured versus Unobscured Environments
5.3. Possible Dependence of Environment on Black Hole Mass

6. SUMMARY