iSEDfit is a Bayesian spectral energy distribution fitting code designed to extract the physical properties of galaxies from broadband photometry. The full suite of routines are publicly distributed as part of my impro IDL library.
If you make use of iSEDfit in any publication please use the following citation:
@MISC{2017ascl.soft08029M,
author = {{Moustakas}, J.},
title = "{iSEDfit: Bayesian spectral energy distribution modeling of galaxies}",
keywords = {Software },
howpublished = {Astrophysics Source Code Library},
year = 2017,
month = aug,
archivePrefix = "ascl",
eprint = {1708.029},
adsurl = {http://adsabs.harvard.edu/abs/2017ascl.soft08029M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}