Key points are not available for this paper at this time.
We present the Edinburgh–Durham Cluster Catalogue (EDCC) is presented. This is the first machine-based, objectively selected sample of clusters of galaxies. It consists of 737 clusters or groups of all richnesses, over 0. 5 sr of sky, centered on the South Galactic Pole (SGP). The primary galaxy dataset for the cluster survey is the Edinburgh–Durham Southern Galaxy Catalogue (EDSGC). The EDCC was constructed using an automatic peak-finding algorithm and is complete to |m₁₀ (b_ j) = 18. 75|. In a comparison with the Abell clusters in the same region 80 percent of their rich clusters nominally brighter than the completion limit are found in addition to many new systems. This suggests that the EDCC is 90 per cent complete for Abell-type clusters. We also conclude that the Abell magnitude system is biased towards bright magnitudes for most of their clusters, and that their richness estimates are prone to a larger uncertainty than they suggest. The EDCC therefore supersedes the Abell catalogue as a data base for statistical studies of cluster properties.
Lumsden et al. (Tue,) studied this question.