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Fig. 5.


Top: projected cumulative mass profiles, as a function of the projected distance from BCGs, corresponding to previous and current lens models for each cluster. The colored regions encompass the 16th and the 84th percentiles; colored solid lines are the median values. The dashed green lines correspond to the mass component associated to cluster members (i.e. sub-halos) from the new lens models with kinematic prior (16th, 50th, 84th percentiles). The multiple image projected distances from the cluster centers are marked with vertical black lines. Bottom: relative variation of the cumulative projected total masses with respect to our reference (green) model.

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