Fig. 1.
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Sample distributed along the star-forming main sequence at z ∼ 3 color-coded by EW([OIII]). The 2D histogram corresponds to the VANDELS parent sample at the same redshift range, and the dashed black line is the main sequence according to Santini et al. (2017). The magenta crosses and cyan triangles are reference samples at low (Berg et al. 2022) and intermediate redshifts (Maseda et al. 2017; Tang et al. 2021), respectively (see Sect. 3.1).
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