Average cluster matter profiles ΔΣ(R) in the Magneticum simulation at five redshifts (color-coded on left) for the same halo-mass bin, 14.65 <  log(M_200c/M_⊙)< 14.85, and for three mass and redshift bins (color and line-type coded on right). The dependence of the matter profiles on cluster mass and redshift is clearly visible. The thickness of the lines represents the 68% credible region in the average matter profiles.