1. INTRODUCTION

2. SAMPLE SELECTION
2.1. The Parent AGN Sample
2.2. AGN Pairs
2.3. AGN Pairs with Tidal Features
2.4. Selection Incompleteness

3. RESULT: THE FREQUENCY OF AGN PAIRS WITH 5 h₇₀⁻¹ KPC ≲ R_P < 100 h₇₀⁻¹ KPC AT Z ~ 0.1

4. DISCUSSION
4.1. Implications for AGN Pairs with Smaller Separations
4.2. Comparison with Binary Quasars
4.3. What Fraction of Moderate-luminosity AGNs Are Triggered in Galaxy Interactions?

5. SUMMARY