Comparison of SFRs derived from radio emission with those derived using other methods. The comparison includes SFRs estimated from Wuyts et al. (2008, green), deblended FIR fluxes from Jin et al. (2018, red), SFRs derived with LEPHARE as in COSMOS2020 ((Weaver et al. 2022), blue), and SFRs scaled from overall average SEDs of the protoclusters to dust continuum (black). Only galaxies with S/N_3GHz > 3 are shown. The black solid line represents a 1:1 relation, while the shaded region indicates the 0.2 dex uncertainties. The dashed colored lines show the median ratios between SFR_radio and the SFRs derived from the fours different methods, respectively: 0.90, 1.81, 0.37, 1.57.