Lensing analysis. Left: projected lensing mass density profile as a function of radius from the PIEMD+eNFW κ-map Zitrin et al. (2015) lens model (black points). Also shown are our best-fit projected NFW profile and 1σ uncertainties (red line and shaded area). The 2D sky angular separation from the cluster center has been converted to radial distance (in Mpc) using the angular distance at the cluster redshift. Right: 2D and 1D posterior probability distributions for the c₂₀₀ and r_s parameters of the 3D mass profile as obtained from the MCMC analysis.