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Fig. 18


Distributions of the starting times of the best fitted SFHs for our sample. The red solid histogram corresponds to the high mass half of the sample, and the blue dashed one to the low mass. The times are defined as the time of observation minus the age of the modeled SED (Eq. (4)). We can see that there are significantly fewer low mass galaxies in the first two Gyr of time.

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