|
par1 | mass, black hole mass in solar masses |
par2 | dist, comoving (proper) distance in Mpc |
par3 | , Eddington ratio |
par4 | , dimensionless black hole spin |
par5 | , coronal radius in marking the transition from (colour temperature corrected) blackbody emission to a Comptonised spectrum. If this parameter is negative then only the blackbody component is used. |
par6 | , log of the outer radius of the disc in units of ; if this is -ve the code will use the self gravity radius as calculated from Laor & Netzer (1989) |
par7 | , electron temperature for the soft Comptonisation component (soft excess) in keV |
par8 | , pptical depth of the soft Comptonisation component. If this parameter is negative then only the soft Compton component is used. |
par9 | , spectral index of the hard Comptonisation component (“power law”) which has temperature fixed to 100 keV. |
par10 | , fraction of the power below which is emitted in the hard comptonisation component. If this parameter is negative then only the hard Compton component is used. |
par11 | Redshift |
norm | K, must be frozen |
Parameters in optxagn:
par1 | mass, black hole mass in solar masses |
par2 | dist, comoving (proper) distance in Mpc |
par3 | , Eddington ratio |
par4 | , dimensionless black hole spin |
par5 | , coronal radius in marking the transition from (colour temperature corrected) blackbody emission to a Comptonised spectrum. If this parameter is negative then only the blackbody component is used. |
par6 | , log of the outer radius of the disc in units of ; if this is -ve the code will use the self gravity radius as calculated from Laor & Netzer (1989) |
par7 | , electron temperature for the soft Comptonisation component (soft excess) in keV |
par8 | , pptical depth of the soft Comptonisation component. If this parameter is negative then only the soft Compton component is used. |
par9 | , spectral index of the hard Comptonisation component (“power law”) which has temperature fixed to 100 keV. |
par10 | , fraction of the power below which is emitted in the hard comptonisation component. If this parameter is negative then only the hard Compton component is used. |
par11 | , colour temperature correction to apply to the disc blackbody emission for radii below with effective temperature |
par12 | , effective temperature criterion used as described above (in K). |
par13 | Redshift |
norm | K, must be frozen |
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Last modified: Friday, 23-Aug-2024 13:20:40 EDT