1. Introduction
2. Catalogue creation
2.1 Image selection
2.2 Full-sensitivity images
2.3 Source finding and measuring
2.4 Merging source-lists and duplicate removal
3. The catalogues
3.1 The primary catalogue
3.2 Auxiliary fixed-resolution, 25-arcsec catalogue
3.3 Auxiliary time-domain catalogue
4. Analysis of the catalogues and images
4.1 Overall noise properties
4.2 Classical source confusion
4.3 Source density
4.4 The fraction of unresolved sources
4.5 Reliability
4.6 Completeness
4.7 Source counts
4.8 Matching to external catalogues
4.9 Photometry
4.10 Astrometry
4.11 RACS-mid and other ASKAP surveys
4.12 The brightness scale of the full-sensitivity images
5. Data availability
6. Summary