Class P09Model

source code

StellarPopulation --+
                    |
                   P09Model

This class describes a Percival et al 2009 (BaSTI; http://albione.oa-teramo.inaf.it) stellar population model. We assume that the synthetic spectra for each model are unpacked under the directory pointed to by fileName.

The wavelength units of SEDs from P09 models are converted to Angstroms. Flux is converted into units of erg/s/Angstrom (the units in the BaSTI low-res spectra are 4.3607e-33 erg/s/m).