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Fig. 7


Mass-richness relation for clusters in common between AMASCFI (at SN > 4 and z < 0.7) and either the Gozaliasl et al. (2014) or Mirkazemi et al. (2015) catalogues. The mass M200 of the X-ray detected clusters was obtained applying the Kettula et al. (2015) M200LX scaling relation. The fitted relation is shown at the top of the figure. The solid black line is the median relation, while the blue zone shows the 68% confidence on the fit parameters. The dashed lines show the intrinsic scatter in the relation.

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