The code SED3FIT (Berta et al. 2013a) performs galaxy SED fitting with a combination of three components: stellar emission; dust emission from star formation; and a possible dusty torus/AGN. The stellar and dust emission are linked by energy balance. Torus emission is simultaneously - but independently - included.

The current implementation adopts Bruzual & Charlot (2003) stellar libraries, Da Cunha et al. (2008) IR-dust libraries, and Feltre et al. (2012) torus+disc models. Some components are to be externally retrieved (see Read-Me file).

Contact: Stefano Berta - stefano.berta [at]