Fig. 1.

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Measurement comparisons of SFR obtained by SED-fitting with the CF00 and C00 attenuation law for the parent sample of 1755 galaxies at 3 < z < 4 taken from the Gómez-Guijarro et al. (2023) photometric catalog. The inset shows the comparative histograms of the SFR ratio between the UV/NIR SFR obtained via an SED fitting with the CF00 (dark blue) and C00 (light blue) attenuation law and the SFRtot = SFRUV + SFRIR. The UV/NIR data come from JADES and SFRtot from the GOODS-ALMA 2.0 catalog. For each distribution, the median value (filled circle) along with its associated 16% and 84% percentiles (segments) are displayed. The red dotted vertical line indicates the benchmark whereby 100% of the total SFR is retrieved by the UV/NIR SED fit.
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