Open Access

Fig. 17.


Fraction of stellar mass in stellar clusters as a function of galaxy stellar mass at different redshifts as indicated in the panel. The solid lines indicate the mean values, and the 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 sampled values. Galaxies at high redshift are more clumpy than at low redshift at fixed stellar mass.

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