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We present optical and near-infrared archival observations of eight edge-ongalaxies. These observations are used to model the stellar content of eachgalaxy using the FitSKIRT software package. Using FitSKIRT, we canself-consistently model a galaxy in each band simultaneously while treating fordust. This allows us to accurately measure both the scale length and scaleheight of the stellar disc, plus the shape parameters of the bulge. Bycombining this data with the previously reported integrated magnitudes of eachgalaxy, we can infer their true luminosities. We have successfully modelledseven out of the eight galaxies in our sample. We find that stellar discs canbe modelled correctly, but have not been able to model the stellar bulgereliably. Our sample consists for the most part of slow rotating galaxies, andwe find that the average dust layer is much thicker than what is reported forfaster rotating galaxies.

The Shape of Dark Matter Haloes IV. The Structure of Stellar Discs in Edge-on Galaxies