Fig. 15.
Variation of the IRX–β relation with redshift, from z = 1.5 to z ≃ 6.0. For each redshift, medians trends are shown with thick colored lines. Observational trends coming from Heinis et al. (2013) and Meurer et al. (1999) are shown with dashed and solid black lines, respectively. The Colored points (according to the redshift color coding) indicate the recent measurements performed by Koprowski et al. (2018) with ALMA.
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