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Fig. 3

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Comparison of inferred galaxy properties (stellar mass, M*, and SFR, color-coded by the dust attenuation parameter, AV) when adopting one of the empirical curves as a dust law and with the fiducial dust attenuation curve for the three sources. The derived properties of the s00717, s01143, and s01149 galaxies are shown on the left, middle, and right panels, respectively. The relative variation in parameters inferred adopting the Calzetti, the SMC, and MW curves with the fiducial curve are represented as circle, square, and diamond, respectively.

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