Fig. 12.

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Fraction of galaxies in each density bin for each Type profiles for the different Hubble morphological type: one corresponds to spirals (darkblue), zero to S0/spiral intermediates (cyan), and minus one to confirmed S0 galaxies (green). Error bars represent the 1σ binomial uncertainties calculated as , where f is the measured fraction and N is the total number of galaxies in the corresponding bin.
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