Cumulative mass and mass fraction profiles of the cluster components out to a projected radius of 350 kpc. Left panel: cumulative two-dimensional mass profiles for all baryonic and dark components of AS1063. The total mass profile and those of the diffuse DM haloes and DM sub-haloes obtained from the model in B19, which differ from ours, are represented with dashed lines. Right panel: cumulative stellar-, gas-, and baryonic-to-total mass fractions from our model. The value of the cosmological baryon fraction from the Planck Collaboration VI (2020) is also shown.