Fig. 13
Galaxies belonging to structures as detected by the Voronoi Tessellation and Percolation technique. The algorithm is run on the sample of likely members with i′ < 21.5 extracted from the Subaru photometric catalog (see text). Open squares, open circles, crosses, and solid circles indicate galaxies in structures at the 95%, 98%, 99%, and 99.9% c.ls., respectively.
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