1. Introduction
2. Observations
3. Data Analysis
3.1. Data Reception and Standard Pipeline Processing
3.2. Astrometric Corrections and Data Preparation
3.3. Source Detection
3.4. Forced Photometry
3.5. The Catalogues
4. Characterisation of the Source Detection Procedure and Catalogue Properties
4.2. Aperture Photometry and Number Counts
5. Conclusions