Constraints on the star-formation rate of z ~ 3 LBGs with measured metallicity in the CANDELS GOODS-South field

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Fig. 6

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Lower panel: ΔE(B − V) vs. Age applying the modified β − A₁₆₀₀ relation in Eq. (1). Upper panel: SFR_fit/SFR_UV vs. Age after applying dust correction inferred from Eq. (1) and the median L_UV-SFR conversion factor for the objects in our sample.

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