Two new sets of models are now available through the XSPEC extra models page (http://heasarc.gsfc.nasa.gov/docs/xanadu/xspec/newmodels.html)
logpar and eplogpar are power-laws whose indices have a log parabolic energy dependence. These models are widely used in blazar research.
optxagnf and optxagn are models for AGN which combine a colour temperature corrected disc and energetically coupled Comptonisation.
Thursday, July 28, 2011
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