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Fig. 9


Two of the most non-Gaussian clusters in our sample. Upper row: the cluster 34726 (Abell cluster A2028). Lower row: the cluster 914 (A1750). From left to right: the DS test bubble plot (here symbol sizes are proportional to the eδ), and RA vs. Dec, and RA vs. velocity (in 102 km   s-1) plots; the symbols show different components as found by Mclust. The star marks the location of the main galaxy.

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