Commit bf818b57 authored by Guang's avatar Guang

change XRB gamma from 2 to 2.5 (Wu et al. 2008)

parent 645891fa
......@@ -58,7 +58,6 @@ class Xray(SedModule):
self.lam_10keV = lam_10keV
lam_100keV = c*cst.h / (1e5*cst.eV)
# Define frequency corresponding to 2 keV in units of Hz.
nu_0p5keV = c / lam_0p5keV
nu_2keV = c / lam_2keV
# We define the wavelength range for the non thermal emission
......@@ -73,9 +72,9 @@ class Xray(SedModule):
# also have two components:
# 2.1 high-mass X-ray binaries (HMXB)
# 2.2 low-mass X-ray binaries (LMXB)
# Assuming gamma=2 for both components (Lehmer et al. 2016)
# Assuming gamma=2.5 for both components (Wu et al. 2008)
# normalized such that L(2-10 keV) = 1.
self.lumin_xrb = self.wave**-1 / np.log(5)
self.lumin_xrb = self.wave**-0.5 / (2*lam_2keV**0.5 - 2*lam_10keV**0.5)
# We compute the unobscured AGN corona X-ray emission
# The shape is power-law with high-E exp. cutoff
......
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