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Fig. 7.


Left panel: sample of 179 star-forming galaxies observed with MUSE, plotted on the M*-SFR plane. The symbols indicate the field and colour indicates the redshift. The dashed lines show a constant sSFR, which is equivalent to a linear relationship: SFR ∝ M*. The red curve shows the model of the star formation sequence from Whitaker et al. (2014) for 0.5 <  z <  1.0. The vertical grey dashed line indicates the selection for the low-mass fit (Sect. 5.2). Right panel: same as the left panel but with the data points removed, showing (the evolution of) the star formation sequence as seen by MUSE, according to Eq. (11).

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