Left: histogram of SFR derived from aperture Hα fluxes, and that estimated from LePhare SED fitting. Right: comparison between the Hα and SED-fitting SFRs, colour-coded by galaxy stellar mass. The black dashed line is the one-to-one correlation. The plot also shows the typical error on the SFR from LePhare (horizontal black error bar, calculated using the SFR_INF and SFR_SUP released in the catalogue) and on the Hα SFR (considering a typical uncertainty of 10% on the flux measurement, see Wisnioski et al. 2019).