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Fig. 5

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Spectral energy distribution of SMM J0658. The solid line corresponds to the best-fit model of Eq. (2)to the long-wavelength points (λ ≥ 250   μm), with β = 1.5, and the shaded area is the 95% confidence interval. The black curve is the LIRG template with far-infrared luminosity 2 × 1011   L from Rieke et al. (2009), magnified by a factor μAB = 100. The data points were taken from Rex et al. (2010) (PACS and SPIRE), this work (SABOCA), Johansson et al. (2011) (LABOCA) and Wilson et al. (2008) (AzTEC).

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