Notes. For each model, the first line specifies the mass components accounted by the cluster-sized halo, parameterized as a NFW distribution.``All'' refers to a mass model (DM+baryons) with a single NFW component. The other models may have additional components either for the gas or the galactic halos. The BCG is either scaled as the other galaxies (``All galaxies'') or embedded in the cluster-zised halo (halos ``with BCG''). The ICM is either modelled apart or embedded in the cluster-sized halo (``Halo with ICM''). The orientation angle is measured north over east and ( ) is the projected length scale (core radius) for the NFW () profile. Parameters in squared brackets were kept fixed in the lensing analysis. Convergences are normalised to the E system source redshift.