1. Introduction

2. Identifying Very Metal-Poor Stars in the RAVE Survey
2.1. The RAVE Survey
2.2. Isolating candidate Very Metal Poor Stars in RAVE

3. Derivation of [Fe/H] Abundances

4. The Stellar [Fe/H] Abundance Distribution Function at low metallicity
4.1. Distribution Function Completeness
4.2. The low metallicity tail of the distribution function

5. Conclusions