Fig. 2.

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Scaling relations between the Sérsic index n, the effective radius Re, the central surface brightness μ0, mean effective surface brightness within Re, ⟨μe⟩, the mass log10(M*/M⊙) and the total magnitude IE of galaxies measured using AutoProf/AstroPhot. The blue distribution shows the probability density function for the 102 cluster member bright disc galaxies while red dots are for cluster member bright ellipticals. The surface brightness is given in mag arcsec−2. The panels on the top and side provide the normalised histograms of the parameters for discs (in blue) and for ellipticals (in red).
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