Fig. 8.

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AFUV − Mstar diagram at z ∼ 4.5 (left) and z ∼ 5.5 (right). The gray areas correspond to the expected relation at z = 4.5 and 5.5 from Bogdanoska & Burgarella (2020). This relation was formed by a broken line, which is flat at log10Mstar ≤ 9.8 and rises at log10 (Mstar) > 9.8. The ALPINE data are very dispersed at z ∼ 4.5, while this flatness is supported by the data at z ∼ 5.5. The conversion from IRX to AFUV is from Burgarella et al. (2005): AFUV = −0.028[log10 (IRX)]3 + 0.392 [log10 (IRX)]2 + 1.094 [log10 (IRX)] + 0.5.
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