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Fig. 7.

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Star-formation rate versus stellar mass diagram. The dashed line corresponds to the Schreiber et al. (2015) curve evaluated at a median sample redshift of z = 1.5. The propagated error dispersion from the fitted errors of the function and a 0.3 dex scatter usually found for the relation in literature are shown as shades. Objects are color-coded by the mass fraction of the late burst population (fburst). Galaxies four times above the main-sequence (black solid line) are consistent with a SED validated starburst population (fburst ∼ 0.1) within the 1σ dispersion shown as green shade area. Bayesian error for SFR and stellar mass are reported.

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