Fits of our model to the XMM‐Newton observations of MCG −6‐30‐15 (Wilms et al. 2001) and to the ASCA observations of GRO J1655−40 (Miller et al. 2004a). For MCG −6‐30‐15, we fit the continuum with a power law of index 1.8 and compare the residuals with the pure scattering model. For this model the best‐fit parameters that we found are ﹩E_{0}=6.51﹩ keV, ﹩kT_{e}=0.1﹩ keV, ﹩\tau =1.2﹩, and ﹩\beta =0.02﹩. Primary photons are generated at the bottom of the outflow (illumination of outflow from inside). For GRO J1655−40 we found the best‐fit parameters ﹩E_{0}=7.1﹩ keV, ﹩kT_{e}=0.1﹩ keV, ﹩\tau =2.0﹩, and ﹩\beta =0.1﹩.