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Star formation rate as a function of stellar mass for the HRS galaxies. Grey dots represent late-type HRS galaxies. Squares show the HRS quenched sources studies in this work; their position relative to the star-forming MS of galaxies before their quenching is marked by grey symbols. Their evolution since quenching is indicated by the triangles coloured according to their agetrunc. For comparison, the MS of Schreiber et al. (2015) at z = 0 is shown as a solid black line along with its dispersion (shaded grey region).
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