
We present a method to model the two-dimensional light distribution of Quasar and Seyfert 1 host galaxies by multi-component fitting. The method has been tested on a large set of simulations, showing its ability to recover total fluxes and morphological properties within the observational errors. We describe the current applications for several well-defined AGN samples
Institut für Physik und Astronomie
Institut für Physik und Astronomie
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