1. INTRODUCTION

2. SAMPLE AND MEASUREMENTS
2.1. The MOSDEF Survey
2.2. X-ray AGN Selection
2.3. IR AGN Selection
2.4. Spectroscopic Data and Optical AGN Selection
2.5. Stellar Mass and SFR Estimates
2.6. [O III] Luminosity as a Proxy of AGN Activity

3. RESULTS
3.1. The Relationship between X-ray and Optical Emission
3.2. AGN Luminosities and Specific Accretion Rates
3.3. AGN Host Galaxy Properties
3.4. The Relationship between Star Formation and AGN Activity

4. DISCUSSION
4.1. Uniqueness and Overlap of AGN Identified at Different Wavelengths
4.2. AGN Selection Biases
4.3. MOSDEF Host Galaxy Properties Compared to the Literature
4.4. Are the Growth of Black Holes and the Growth of their Host Galaxies Correlated at z~2?

5. SUMMARY