Fig. 6.
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Updated star formation rate as a function of stellar mass colour-coded by λR. The grey-shaded region in the background corresponds to the 3D-HST sample measurement. The dotted and dashed white lines indicate the star formation main sequence for Universe ages of 12.4 Gyr (z = 0.1) and 6.8 Gyr (z = 0.8), respectively, from Eq. (1) of Whitaker et al. (2012). The colour map shows a LOESS-smoothed version of the markers on top. The dots and triangles represent seeing-corrected and uncorrected values, respectively. This figure corresponds to the updated version of Figure 9 in Muñoz López et al. (2024).
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