1. Introduction

2. XMM-Newton data reduction

3. Source detection
3.1. Source list generation
3.2. Growth curve analysis
3.3. Physical parameter estimation

4. Photometric redshift estimation
4.1. Spectroscopic redshifts
4.2. Comparison of spectroscopic and photometric redshifts

5. Results
5.1. Galaxy cluster sample
5.2. Survey sky-coverage
5.4. Cross-correlation with known sources
5.5. Cross-correlation with the Southern Cosmology Survey clusters

6. Discussion
6.1. Error budget of the X-ray analysis
6.2. Project outlook

7. Summary and conclusions