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Fig. 5.

Fig. 5. Refer to the following caption and surrounding text.

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SFE as a function of gas fraction (fgas) for PP, NP, and PN galaxies in the low-mass (upper panel) and high-mass (lower panel) bins. All parameters are expressed relatively to those of NN galaxies at a given M. The coloured map represents the normalised SFR, while green borders around the data points highlight galaxies that increased their stellar mass by more than 25% within 2.5 Gyr (τ25 < 2.5 Gyr). The percentages of each galaxy type within each quadrant are included.

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