1 INTRODUCTION

2 BACKGROUND
2.1 The kinematic template
2.2 The chemical template

3 OBSERVATIONAL DATA

4 THE DYNAMICAL ANALYSIS
4.1 VISTA vs. 2MASS magnitudes
4.2 Absolute magnitudes and ages
4.3 Distances, kinematics, and orbital parameters
4.4 Aside: the Gaia-ESO selection function

5 HUNTING FOR SUBSTRUCTURE
5.1 Abundance trends of the low J_z/J_c stars
5.2 Identifying substructure in J_z/J_c
5.3 Characterizing the accreted population

6 MEAN MASS OF THE MERGING SATELLITE(S)

7 THE QUIESCENT MILKY WAY

8 CONCLUSIONS AND FUTURE PROSPECTS