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Fig. A.1.
Histogram of the 
values (see Eq. (2)) for the quiescent sample (intrinsic red galaxies) at different redshifts using the BC03 SSP models. Solid lines illustrate the MLE best fit of the 
distribution at different redshifts. Dashed coloured lines show the upper 3σ limit of the distributions provided by the MLE method.
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