Fig. 8.
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Number of SFEs as a function of the stellar mass. The violins show the mass distribution with the number of galaxies displayed at the top of each set. Black lines correspond to the mean of each distribution. The majority of galaxies with one SFE have SFR described by one exponential function. Higher numbers of SFEs are mostly modelled by exponential and Gaussian distributions. In Appendix A.6 we present some examples of galaxies with different SFEs.
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