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Fig. 3.

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Corner-plot posterior distributions for the parameters used in the dust SED modeling: the dust temperature, Tdust; the observed solid angle of the emitting region, Ωs; the mass of dust, Mdust; and the dust emissivity index, β. In the corner plots, darker points show values corresponding to higher posterior probabilities. We also show the marginalized posterior distributions for the dust optical depth at the frequency of [C II], τ1900 GHz; and of the infrared luminosity, LIR. In all the marginalized distributions, the median values are marked with a dashed line, and the values corresponding to the 1-σ confidence intervals are marked with dotted vertical lines.

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