Fig. 17.
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Attenuation–M* relation (top panel) and the SFR–M* relation (bottom panel) derived from the EWS-SFsim stacked mock spectra. The attenuation is measured using the Balmer decrement (Hα/Hβ ratio), whilst the SFR is calculated from the dust-corrected Hα luminosity, applying the Calzetti et al. (2000) extinction law and assuming case B recombination conditions (electron density of 100 cm−2 and temperature of 10 000 K. The panel layout follows the structure of Fig. 14. Shaded regions represent the 1σ uncertainties in the measured quantities.
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