1 INTRODUCTION

2 OBSERVATIONS
2.1 Photometry from SkyMapper
2.2 Medium resolution spectroscopy with AAOmega on the AAT
2.3 High resolution spectroscopy with MIKE on Magellan

3 ANALYSIS
3.1 Data Reduction and Radial Velocities
3.2 Atmospheric Parameters
3.3 Chemical Abundances
3.4 Distances to the stars

4 ANALYSIS OF PREVIOUSLY STUDIED STARS

5 RESULTS AND DISCUSSION
5.1 Positions and Kinematics
5.2 Stellar Parameters
5.3 Chemical Abundances

6 CONCLUSIONS