1. Introduction

2. The optical survey

3. The UKIDSS GCS infrared survey

4. Cross-matching with optical data
4.1. Revised membership of optically selected candidates
4.2. New cluster member candidates
4.3. Radial distributions
4.4. Proper motions for the brightest member candidates
4.5. Fainter cluster member candidates

5. The luminosity and mass functions
5.1. The luminosity function
5.2. The mass function

6. Conclusions and future work