1 INTRODUCTION

2 SAMPLE SELECTION AND DATA
2.1 Sample selection
2.2 Strong Lensing
2.3 Gas kinematics
2.4 Bulge and disk structural parameters
2.5 Stellar Population Synthesis Masses

3 REFERENCE MASS MODEL
3.1 Overview
3.2 Constraints and priors

4 RESULTS
4.1 Is the IMF universal within individual galaxies?
4.2 Are disks sub-maximal?
4.3 Are dark matter haloes cuspy?

5 TESTING SYSTEMATIC EFFECTS
5.1 Alternative dark matter halo models
5.2 Line of sight effects
5.3 Cold Gas

6 SUMMARY