
par1  kTs, temperature of the seed blackbody spectrum (keV) 
par2  gamma, when it is set = 3 the seed soft spectrum is a blackbody, otherwise it approximates a modified blackbody 
par3  kTe, electron temperature of the subrelativistic outflow (keV) 
par4  tau, radial optical depth of the subrelativistic outflow 
par5  beta, bulk outflow velocity of the thermal electrons 
par6  fbflag, if set = 0 only the firstorder bulk Comptonization term is considered, if set = 1 also the secondorder term is computed, where 
par7  log(A), geometrical covering factor which determines the relative weights of the seed and comptonized spectra to the total flux 
par8  z, redshift 
par9  a_boost, energy index of the Green's function with which the formerly comptonization spectrum is convolved 
norm  , where is the apparent blackbody radius in units of cm and is the sorce distance in Mpc 
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Last modified: Tuesday, 28May2024 10:09:22 EDT