1. INTRODUCTION

2. CLUSTER SAMPLE

3. OBSERVATIONS AND DATA REDUCTION
3.1. LABOCA 870 µm observations
3.2. ATCA 2.1 GHz observations
3.3. Herschel observations

4. COMPLEMENTARY DATA
4.1. Spitzer/IRAC data
4.2. Optical data

5. SOURCE EXTRACTION AND PHOTOMETRY

6. ANALYSIS OF 870 µm POINT SOURCES
6.1. Counterpart identification
6.2. SED Modeling and Photometric Redshifts
6.4. Number counts

7. CONCLUSIONS