1. INTRODUCTION

2. RESEARCH METHODOLOGY

2.1. Connecting halos to galaxies and BHs

2.3. Input Eddington ratio distribution

2.5. The $Q$ parameter

3. OUTPUTS

4.2. AGN Large-scale bias

5. ADDITIONAL DEPENDENCIES IN THE INPUT MODEL PARAMETERS

6. HOW TO BUILD REALISTIC AGN MOCKS

7. DISCUSSION

8. CONCLUSIONS