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Fig. 2


Relation between dust attenuation and stellar mass for our stacked galaxies over 0.02 ≲ z ≲ 3.0, with the color code shown in the top-left corner. The dust attenuation was derived with the LIR/LUV ratio and the calibration of Buat et al. (2005). For reference, we represent the local relation as reported in Sobral et al. (2012) with a solid dark gray curve and the relation at z ~ 1.5 presented in Heinis et al. (2014) with a light gray solid line.

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