1 INTRODUCTION

2 LINE-DETECTION LIMITS

3 SFR FUNCTIONS AND REDSHIFT DISTRIBUTIONS

4 STRONGLY LENSED GALAXIES

5 UNLENSED GALAXY POPULATIONS

6 COMPARISON AND SYNERGIES WITH OTHER LARGE-AREA SURVEYS

7 REVEALING GALAXY PROTO-CLUSTERS VIA DUSTY STARBURSTS

8 COMPARISON WITH OTHER LARGE-AREA CLUSTER SURVEYS

9 CONCLUSIONS