1. INTRODUCTION

2. THE RASS AGN-LRG CCF MEASUREMENTS

3. MODELING THE HALO OCCUPATION DISTRIBUTION

3.1. Model Ingredients

4. RESULTS FROM THE HOD MODELING

4.1. Fit Results

4.2. HODs and Space Densities

4.3. Effects of Central AGNs

5. DISCUSSION

5.1. Comparison with Results from Paper I

5.2. Implications for the Environments of AGN Accretion

6. CONCLUSION