
par1  a/M; BH angular momentum (GM/c) 
par2  theta_o; observer inclination (0 = pole on, degrees) 
par3  rin; inner radius (GM/c) 
par4  ms; 0 means integrate from rin, 1 means integrate emission from above the marginally stable orbit only 
par5  rout; outer radius (GM/c) 
par6  alpha; accretion disk emissivity scales as for 
par7  beta; accretion disk emissivity scales as for 
par8  rb; boundary radius between inner and outer emissivity laws (GM/c) 
par9  zshift; overall Doppler shift 
par10  limb; 0 means isotropic emission, 1 means Laor's limb darkening (), 2 means Haardt's limb brightening ( 
par11  ne_loc; number of grid points in local energy (energy resolution of local flux, the grid is equidistant in logarithmic scale) 
par12  normal; 0 means normalize total flux to unity, +ve value means normalize to unity at the energy given by the parametervalue, ve value means unnormalized. 
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Last modified: Tuesday, 28May2024 10:09:22 EDT