Figure 5From: A detection metric designed for O’Connell effect eclipsing binariesThe phased light curves of the discovered OEEB data from Kepler, clustered via k-mean applied to the DF feature space. Cluster number used is based on trial and error, and the unsupervised classification has been implemented here only to highlight morphological similarities. The top four plots represent clusters 1–4 (left to right), and the bottom four plots represent clusters 5–8 (left to right)Back to article page