Fig. C.1.
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⟨ t⋆ ⟩M, log M⋆, SFR, and AV of clumps and complexes plotted against the normalized log distance log d/Re to the center of the host galaxy. Each column of panels corresponds to a different galaxy. Top panels show data for Hα clumps (gold), middle panels show F275W clumps (pink) and bottom panels show star-forming complexes (purple). Black dashed lines show linear fits to the relations. For SFR and AV we use the same selection as in Fig. 6.
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