Fits of our model to the XMM‐Newton observations of MCG −6‐30‐15 and to the ASCA observations of GRO J1655−40 using the model for which the photoabsorption along with scattering are included. For MCG −6‐30‐15, the best‐fit model parameters that we found are ﹩E_{0}=6.51﹩ keV, ﹩kT_{e}=0.1﹩ keV, ﹩\tau =1.7﹩, and ﹩\beta =0.02﹩. For GRO J1655−40, we found the best‐fit parameters ﹩E_{0}=7.1﹩ keV, ﹩kT_{e}=0.1﹩ keV, ﹩\tau =3.3﹩, and ﹩\beta =0.25﹩.