bexriv: reflected e-folded broken power law, ionized medium
Broken power-law spectrum multiplied by exponential high-energy cutoff, , and reflected from ionized material. See Magdziarz & Zdziarski 1995, MNRAS, 273, 837 for details. Ionization and opacities of the reflecting medium is computed as in the procedure absori. The output spectrum is the sum of an e-folded broken power law and the reflection component. The reflection component alone can be obtained for . Then the actual reflection normalization is . Note that you need to change then the limits of excluding zero (as then the direct component appears). If , there is no cutoff in the power law. The metal and iron abundances are variable with respect to those set by a command abund. Send questions or comments to aaz@camk.edu.pl .
par1 |
, first power law photon index |
par2 |
Ebreak, break energy (keV) |
par3 |
, second power law photon index |
par4 |
Ec, the e-folding energy in keV (if there is no cutoff) |
par5 |
relrefl, reflection scaling factor (1 for isotropic source above disk) |
par6 |
redshift, z |
par7 |
abundance of elements heavier than He relative to the solar abundances |
par8 |
iron abundance relative to the above |
par9 |
cosine of inclination angle |
par10 |
disk temperature, K |
par11 |
disk ionization parameter, , where Fion is the 5eV–20 keV irradiating flux, n is the density of the reflector; see Done et al., 1992, ApJ, 395, 275} |
norm |
photon flux at 1 keV of the cutoff broken power-law only (no reflection) in the observed frame.} |