SFMS and MZR measured from the most recent values of the SFHs and the [Z/H] we employed (∼20 Myr) obtained from full spectral fitting. The full distribution (ALL) is shown as black points, with MS (blue) and RET (brown) shown in colored points in the left and right columns, respectively. The contours follow the star-forming subsample as defined in Sect. 3.2, which is used to measure the SFMS and MZR (red lines). In the top two panels we show the SFMS at z ∼ 0 from Speagle et al. (2014, left) and Popesso et al. (2023, right) for comparison with ours.