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Fig. 6.

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Average probability that a galaxy of a given stellar mass with at least one clump hosts either a single clump (continuous lines) or two or more clumps (dashed lines) for starbursts (blue circles), galaxies on the MS (black squares), in the green valley (green diamonds), and in the red sequence (red crosses). For each class, we show the standard deviation of the probability as a semitransparent filled area with a similar color. The probabilities are computed using Eqs. (C.6) and (C.8).

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