Observational and theoretical constraints on the formation and early evolution of the first dust grains in galaxies at 5 < z < 10

Open Access

Fig. B.1.

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Probability Distribution function (PDF) derived from the fit for each of the important parameters for this paper: L_FUV, L_dust, M_dust, Age_main, M_star and SFR for each representative Hi-z LBGs.

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