Mass-richness relation for clusters in common between AMASCFI (at S∕N > 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) M200 −LX 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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