1. INTRODUCTION

2. GALAXY TRACER SETS  
2.1. SDSS Main Galaxy Sample  
2.2. SDSS Luminous Red Galaxy Sample  
2.3. Extended SDSS Luminous Red Galaxy Sample  

3. AGN SAMPLES  
3.1. RASS/SDSS AGN Samples  
3.2. Optically-selected SDSS Samples  

4. CLUSTERING ANALYSIS  
4.1. Inferring the AGN Auto-correlation Function  
4.2. Robustness of the Clustering Measurements  

5. BIAS FROM THE HOD MODELING  
5.1.2. Luminous Red Galaxies ($0.16<z<0.36$)  
5.1.3. Extended LRGs ($0.36<z<0.50$)  
5.3. AGN HOD Bias Results  
5.4. Power Law versus HOD Derived Bias Parameters  

6. DISCUSSION  
6.1. Comparison with X-ray Selected Broad-line AGN Clustering Measurements  
6.2. Optical versus X-ray Selected AGN Clustering Properties  
6.3. Broad-line versus Narrow-line AGNs  
6.4. Impact of Radio-loud Broad-line AGN on the Clustering Signal  
6.5. Luminosity Dependence of the Clustering Signal  
6.6. Current Picture of AGN Clustering  

7. CONCLUSIONS