An Illustration of Modeling Cataclysmic Variables: HST, FUSE, SDSS   Spectra of SDSSJ080908.39+381406.2
  We use FUSE, HST, and SDSS spectra of the cataclysmic variable SDSSJ0809 to illustrate procedures for calculating and testing system models. Our final model has an accretion disk temperature profile similar to the SW Sextantis profile determined from tomographic reconstruction. 
Albert P. Linnell, D.W.Hoard, Paula Szkody, Knox S. Long, Ivan Hubeny,   Boris Gansicke, and Edward Sion