1. Introduction  
2. Data  
3. Methods  
3.1. PZWav algorithm  
3.2. An adaptive membership estimator (AME)  
3.3. Cluster characterisation  
4. PZWav’s Galaxy cluster catalogue  
4.1. Catalogue  
4.2. Cluster member catalogue  
4.3. Group and cluster regimes  
4.4. Generating a refined catalogue using richness  
5. Results  
5.1. Comparisons to AEGIS X-ray catalogue  
5.2. Extended X-ray catalogue  
5.3. Scaling relations  
5.4. Comparisons between optical catalogues  
5.5. Significance of the detection catalogues  
6. Summary and conclusions