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Fig. 8

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SED models of the galaxies M 51, M 83, IC 342 and NGC 3190. The SEDs modelled with submm data are indicated by the black lines. Dashed lines indicates the model obtained when submm data are omitted. Observational constraints are superimposed (filled circles). When the error bars are not shown, the errors are smaller than symbols. The thick orange line shows the IRS spectrum used in the SED modelling when available. The open circles indicate the expected modelled fluxes integrated over the instrumental bands. The green and red lines respectively distinguish the stellar and dust contributions.

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