Home | Trees | Indices | Help |
---|
|
module for performing calculations on Spectral Energy Distributions (SEDs)
(c) 2007-2009 Matt Hilton
This module provides classes for manipulating SEDs, in particular the Bruzual & Charlot 2003 and Maraston 2005 stellar population synthesis models are currently supported. Functions are provided for calculating the evolution of broadband colours and magnitudes in these models with redshift etc.. It is not especially fast at present.
|
|||
Passband This class describes a filter transmission curve. |
|||
SED This class describes a Spectral Energy Distribution (SED). |
|||
VegaSED This class stores the SED of Vega, used for calculation of magnitudes on the Vega system. |
|||
StellarPopulation This class describes a stellar population model, either a Simple Stellar Population (SSP) or a Composite Stellar Population (CSP), such as the models of Bruzual & Charlot 2003 or Maraston 2005. |
|||
M05Model This class describes a Maraston 2005 stellar population model. |
|||
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. |
Home | Trees | Indices | Help |
---|
Generated by Epydoc 3.0.1 on Sun Mar 22 16:49:56 2009 | http://epydoc.sourceforge.net |