SFR–M_* relation at 4 < z < 5. Dark-gray hexagons show the dust-attenuated SFRs (i.e., SFR_IR) inferred by stacking all SFGs with a A³COSMOS coverage, while dark-green hexagons show their total SFRs, i.e., adding the contribution of their unattenuated SFRs measured in the UV (i.e., SFR_UV; symbols are slightly offset along the stellar mass axis for clarity). Light-gray and lime-green circles display the same quantities but for our stacking analysis which excludes the ALMA primary targets (symbols are slightly offset along the stellar mass axis for clarity). The dark-green solid and red dotted lines represent the MS and its ±0.3 dex dispersion from Schreiber et al. (2015), whose normalization happens to be perfectly consistent with our dark-green hexagons, i.e., MS_{All,  Fit} ≡ MS_S15. The lime-green line is obtained by renormalizing the MS of Schreiber et al. (2015) to fit our lime-green circles, i.e., MS_{Offcenter,  Fit} ≡ MS_S15 − 0.3 dex. For each stellar mass bin, we give the fraction of ALMA primary targets and in parenthesis their weights in our stacks. Finally, pink squares and diamonds show the total and dust-attenuated SFRs found in Khusanova et al. (2021) by stacking in three stellar mass bins, ALMA observations of all (detected and undetected) z ∼ 4.5 SFGs from the ALMA ALPINE survey.