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Fig. 9


The cumulated quenched SMF since z = 1.1 in our simple model is compared to the increase in the observed SMF of quiescent galaxies in Ilbert et al. (2010) and Arnouts et al. (2007). The comparison is meaningful only out of the shaded area, on the side indicated by the arrow (the limit corresponds to log (M) = 9.6, the lower stellar mass used in Ilbert et al. (2010) at redshift 1.1, which we use as reference.

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