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Fig. B.6

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(U,V), (V,W) and (U,W) planes (from left to right) of the member candidates to the Pleiades MG, which are selected by means of Monte Carlo simulations. From the second row to the bottom, we display the distribution of good, possible, unlikely and disregarded candidates. The color codes the density level: light pink/purple when the sources are sparsely distributed, to orange/red for a higher density. For comparison purposes, we show the loci of known members taken from Montes et al. (2001) on the first row. We also over-plotted ellipses of three k values, which correspond to the 10% threshold for 1D, 2D, and 3D spatial considerations (Fig. A.2) by dashed, dash-dotted, and solid lines, respectively.

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