CIGALE: Code Investigating GALaxy Emission

Details CIGALE: Code Investigating GALaxy Emission CIGALE: Code Investigating GALaxy Emission

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ascl.soft11004n&link_type=abstract

Astrophysics Source Code Library, record ascl:1111.004

Astronomy and Astrophysics

Astrophysics

Scientific paper

The CIGALE code has been developed to study the evolution of galaxies by comparing modelled galaxy spectral energy distributions (SEDs) to observed ones from the far ultraviolet to the far infrared. It extends the SED fitting algorithm written by Burgarella et al. (2005, MNRAS 360, 1411). While the previous code was designed to fit SEDs in the optical and near infrared, CIGALE is able to fit SEDs up to the far infrared using Dale & Helou (2002, ApJ 576, 159). CIGALE Bayesian and CIGALE Monte Carlo Markov Chain are available.

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