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Fig. 6

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Predicted luminosity of CIII] 1909 Å as a function of the total SFR (SFRUV+IR) for ks = 0.34 (left panel) and ks = 5 (right panel). The colours correspond to 1–2σ dispersion. The central region between the dashed grey lines represents the SFR range of the ALPINE subsample modelled in this work. Red and blue represent the two SFHs considered in this work: continuous and Δtq = 5 Myr. The black points are the observed data from Llerena et al. (2023), the blue points from Markov et al. (2022).

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