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Fig. 4.

Fig. 4. Refer to the following caption and surrounding text.

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Example of FIR SED fitting for one galaxy in our sample. Black points show the observed photometric fluxes as a function of wavelength. The solid blue and purple curves correspond to the best-fit MS and starburst (SB) FIR templates, respectively. The inset shows the posterior marginal likelihood of the FIR luminosity ℒ(LIR) obtained for the MS (blue) and starburst (purple) solutions. Here, we show a case where both the SB-type and MS-type templates provide reasonable fits, with a slight preference for the SB-type.

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