Host Galaxy properties of highly accreting SMBH in the local Universe

An open question in extragalactic astronomy is the extent to which Active Galactic Nuclei (AGN) affect the evolution of their host galaxies. Host galaxy properties of AGN, such as star formation rate and stellar mass, are key parameters for studying the role of AGN in galaxy evolution. However, disentangling the infrared emission from AGN and star-forming components is a challenging task that requires comparing advanced spectral energy distribution (SED) models.