Fraction of galaxies more massive than 10¹⁰ M_⊙ of a given galaxy morphology (see Sect. 3.3) as a function of local density. Errors on the fractions are computed from Poisson statistics. We show as coloured vertical regions the likely association between local density and density regions. We note that we find no significant differences between field-like and filament-like densities. We do find a rise in the fraction of ellipticals and a decline of disc-like morphologies towards the densest regions probed here.