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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 |
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