Fig. 5.

IRX–βUV diagram. Lines show different IRX–βUV relations: the well-known local starburst galaxies calibration (M99; triple-dot-dashed line), the aperture correction of M99 relation by Takeuchi et al. (2012; dashed line), and the relation derived from a FIR stacking analysis over the same LBG sample (AM16; dotted blue line). In addition, we plot the IRX–βUV results from LBGs at redshifts, z ∼ 3 (Koprowski et al. 2018, orange dots) and 2 < z < 3 (Bouwens et al. 2016, gray dots), star-forming galaxies at redshifts, 2 < z < 3 (McLure et al. 2018, green dots) and 1.5 < z < 2.5 (Reddy et al. 2018, black dots), and a mass selected sample at redshift z ∼ 3 (Bourne et al. 2017, blue dots). The downward triangles represent upper limits.
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