Same as Fig. 17: fraction of stellar mass in stellar clusters as a function of galaxy stellar mass at different redshifts as indicated in the panel, except that a lower number of stellar particles are used to detect stellar clumps (10 instead of 50) in AdaptaHOP. The solid lines indicate the mean values, and dashed lines stand for the error on the mean. The data points are overplotted for the most extreme redshifts to appreciate the scatter in the distribution of values.
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