July 12, 2016

The code SED3FIT (Berta et al. 2013a) is now publicly available. It 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).
The SED3FIT package can be downloaded here.
 

For questions, get in touch with Stefano Berta (stefano.berta [at] yahoo.it)