Fig. 4.
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SFR as a function of stellar mass for equilibrium (left) and non-equilibrium (right) galaxies. The solid red line indicates the SFMS from Renzini & Peng (2015), with dashed lines showing the adopted scatter. Colour maps indicate the number of galaxies per bin in each panel; note that the colour scales differ between the equilibrium and non-equilibrium panels, reflecting the different sample sizes.
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