Class BC03Model
source code
StellarPopulation --+
                    |
                   BC03Model
This class describes a Bruzual & Charlot 2003 stellar population 
  model, extracted from a GALAXEV .ised file using the galaxevpl program 
  that is included in GALAXEV. The file format is white space delimited, 
  with wavelength in the first column. Subsequent columns contain the model
  fluxes for SEDs of different ages, as specified when running galaxevpl. 
  The age corresponding to each flux column is taken from the comment line 
  beginning "# Age (yr)", and is converted to Gyr.
  For example, to load a tau = 0.1 Gyr burst of star formation,  solar 
  metallicity, Salpeter IMF model stored in a file (created by galaxevpl) 
  called "csp_lr_solar_0p1Gyr.136":
  bc03model = BC03Model("csp_lr_solar_0p1Gyr.136")
  The wavelength units of SEDs from BC03 models are Angstroms. Flux is 
  converted into units of erg/s/Angstrom (the units in the files output by 
  galaxevpl are LSun/Angstrom).