SLIMBH is a relativistic model for X-ray continuum of stationary slim accretion disks around stallar mass black holes. This model is based on disk radial structure solutions presented in Sadowski et al. 2010 combined with vertical structure computed using TLUSTY code to make the best model for X-ray continuum for a wide range of luminosities up to Eddington limit. See also Straub et al. 2011.
The model requires a FITS table with pre-computed spectral data.
FITS table download link: slimbb-full.fits
The following plot shows a comparison between SLIMBH spectrum (red) and relativistic thin disk spectrum (blue) for a 10 M_Sun black hole with spin a=0.9 and disk luminosity L=0.5 L_Edd.