Extragalactic extinction: Calzetti, Kinney and Storchi-Bergmann
The extragalactic extinction is calculated using the formula from  . This model is intended to be used to modify another model (e.g. by multiplying the two together). It is for use when the independent axis is in Angstrom.
>>> create_model_component("xgal", "mdl") >>> print(mdl)
Create a component of the xgal model and display its default parameters. The output is:
mdl Param Type Value Min Max Units ----- ---- ----- --- --- ----- mdl.ebv thawed 0.5 -3.40282e+38 3.40282e+38
The attribute for this object is:
When evaluated on a binned grid, the lower-edges of the bins are used for the calculation.
-  Calzetti, Kinney, Storchi-Bergmann, 1994, ApJ, 429, 582 http://adsabs.harvard.edu/abs/1994ApJ...429..582C
See the bugs pages on the Sherpa website for an up-to-date listing of known bugs.