
par1  lineE: rest frame line energy (keV) 
par2  Index1: emissivity index for the inner disk 
par3  Index2: emissivity index for the outer disk 
par4  Rbr: break radius separating the inner and outer portions of the disk (gravitational radii) 
par5  a: dimensionless black hole spin 
par6  Incl: disk inclination angle to the line of sight (degrees) 
par7  Rin: inner radius of the disk in units of the radius of marginal stability 
par8  Rout: outer radius of the disk in units of the radius of marginal stability 
par9  z: redshift 
par10  limb: limbdarkening/brightening law with 0=isotropic, 1=darkening (flux 1+2.06mu), 2=brightening (flux ln(1+1/mu)) where mu=cos(emission angle) 
norm  flux in line (photons/cm/s) 
The parameters for rellinelp are :
par1  lineE: rest frame line energy (keV) 
par2  h: height of the primary source (GM/c2) 
par3  a: dimensionless black hole spin 
par4  Incl: disk inclination angle to the line of sight (degrees) 
par5  Rin: inner radius of the disk in units of the radius of marginal stability 
par6  Rout: outer radius of the disk in units of the radius of marginal stability 
par7  z: redshift 
par8  limb: limbdarkening/brightening law with 0=isotropic, 1=darkening (flux 1+2.06mu), 2=brightening (flux ln(1+1/mu)) where mu=cos(emission angle) 
par9  gamma: powerlaw index of the primary source (Egamma) 
norm  flux in line (photons/cm/s) 
and the parameters for rellinelpext are :
par1  lineE: rest frame line energy (keV) 
par2  a: dimensionless black hole spin 
par3  Incl: disk inclination angle to the line of sight (degrees) 
par4  Rin: inner radius of the disk in units of the radius of marginal stability 
par5  Rout: outer radius of the disk in units of the radius of marginal stability 
par6  z: redshift 
par7  limb: limbdarkening/brightening law with 0=isotropic, 1=darkening (flux 1+2.06mu), 2=brightening (flux ln(1+1/mu)) where mu=cos(emission angle) 
par8  gamma: powerlaw index of the primary source (Egamma) 
par9  hbase: lower height of radially extended primary source 
par10  htop: upper height of radially extended primary source 
par11  vbase: velocity of the source at hbase 
par12  v100: velocity of the source at 100 rg above hbase 
norm  flux in line (photons/cm/s) 
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Last modified: Tuesday, 28May2024 10:09:22 EDT