We present CIGALE (Burgarella et al. 2005; Noll et al. 2009), a software developed at the Laboratoire d'Astrophysique de Marseille to fit galaxy spectral energy distributions from the rest-frame far-UV to far-IR wavelength range, and to derive some of their physical parameters. We also give some examples of scientific results obtained with CIGALE.
Cite
@article{arxiv.1111.1117,
title = {CIGALE: Code Investigating GALaxy Emission},
author = {Yannick Roehlly and Denis Burgarella and Véronique Buat and Élodie Giovannoli and Stefan Noll and Paolo Serra},
journal= {arXiv preprint arXiv:1111.1117},
year = {2011}
}
Comments
4 pages, 2 figures, proceeding of a poster to be presented at ADASS XXI in Paris