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            bexriv: reflected e-folded broken power law, ionized medium

Broken power-law spectrum multiplied by exponential high-energy cutoff, exp(-E_c*E), 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 |rel_refl|<0. Then the actual reflection normalization is |rel_refl|<0. Note that you need to change then the limits of |rel_refl|<0 excluding zero (as then the direct component appears). If E_c=0, 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

Gamma_1, first power law photon index

par2

Ebreak, break energy (keV)

par3

Gamma_2, second power law photon index

par4

Ec, the e-folding energy in keV (if E_c=0 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, xi = 4*pi*F_ion/n, 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.}

 

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