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Fig. 3

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Slope, value of best fit line at MV =  −20 and scatter of the median RS values of the 100 Monte Carlo runs for each cluster versus cluster velocity dispersion (σclus, left panels) and cluster X-ray luminosity (LX, right panels). Error bars refer to the error of the median of the 100 simulations. In red (on-line version), clusters whose RS is contaminated by another structure (see text).

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