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Dust energy balance study of two edge on spiral galaxies in the Herschel ATLAS survey

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Table 1. The fundamental properties of the two galax-ies in our sample. Stellar masses, TIR luminosities,dust masses, SFRs and specific SFRs are calculatedusing a MAGPHYS modelling of the SED.
Table 2. Observed flux densities and corresponding errorsfor IC 4225 and NGC 5166.
Table 3. The parameters of the best-fitting models forIC 4225 and NGC 5166. The top 13 parameters with er-ror bars correspond to the FITSKIRT models as described inDG14
Figure 2. The SED of IC 4225 (top) and NGC 5166 (bottom). The coloured dots with error bars correspond to the flux densities listed in Tablelines are the simple models based only on the optical data (Case A), the solid lines are the models in which an addit
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