1 INTRODUCTION

2 THEORY
2.1 Tomographic Signal

3 DATA
3.1 The Deep Lens Survey
3.2 Foreground Lens Selection
3.3 Lyman Break Galaxy Selection

4 RESULTS
4.1 Lyman Break Galaxy Magnitude Bins
4.2 Galaxy-Mass Correlation
4.3 Tomography

5 DISCUSSION AND CONCLUSIONS