Fig. 3.
PDFs of the three free parameters in our model optimisation: the intrinsic FUV luminosity from the young non-ionising stellar component, Lyni, FUV (left), the intrinsic FUV luminosity from the young ionising stellar component, Lyi, FUV (middle), and the total dust mass, Mdust (right). Dashed red lines are the parameter values for the best-fitting model.
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