A modified blackbody disk model. The spectrum from the inner region of an accretion disk where the viscosity is dominated by radiation pressure.
|par1||accretion rate in Eddington Luminosities|
|par2||central mass in solar mass units|
|par3||inner disk radius in gravitational (= 3 Schwarzschild radii)|
|norm||where is the inclination of the disk and is the distance in units of 10 kpc|