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Fig. 2


Relative uncertainty of dust masses (defined as σ(Mdust) /Mdust), based on DL07 SED modeling, as a function of position in the z-M-SFR space. The two diagrams belong to two independent simulations, obtained noise levels of individual detections in GOODS-S and COSMOS, applied to artificial photometry based on the SEDs by Magnelli et al. (2014). For reference, black lines denote the position of the main sequence (MS, solid line) of star formation (Elbaz et al. 2011) and ± 4, ± 10 MS levels (dashed).

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