Same as Fig. 6, but for an AGN (ID = 7) fitted with the “double-powerlaw” model (left) and the “powerlaw + blackbody” model (right), respectively. In addition to the power-law normalization (logPowNorm) and the background normalization (logBkgNorm), for the first model, the spectral shape parameters include the ∆Γ for the additional power-law, the Γ of the primary power-law, the logN_H, and the flux ratio of the secondary to the primary power-law at 1 keV (logFrac); and for the second model, the parameters determining the spectral shape include the Γ of the power-law, the logN_H, the log kT of the blackbody, and the blackbody normalization (logBBNorm).