We present a broadband X-ray analysis of a new homogeneous sample of 95 active galactic nuclei (AGN) from the 22-month Swift/BAT all-sky survey. For this sample we treated jointly the X-ray spectra observed by XMM-Newton and INTEGRAL missions for the total spectral range of 0.5–250 keV. Photon index Γ\documentclass[12pt]{minimal}
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\begin{document}$\varGamma$\end{document}, relative reflection R\documentclass[12pt]{minimal}
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\begin{document}$L_{\mathrm{corr}}$\end{document} are determined for all objects of the sample. We investigated correlations Γ\documentclass[12pt]{minimal}
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\begin{document}$\varGamma$\end{document}–R\documentclass[12pt]{minimal}
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\begin{document}$N_{\mathrm{H}}$\end{document}. Dependence “Γ\documentclass[12pt]{minimal}
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\begin{document}$R$\end{document}” for Seyfert 1/2 galaxies has been investigated separately. We found that the relative reflection parameter at low power-law indexes for Seyfert 2 galaxies is systematically higher than for Seyfert 1 ones. This can be related to an increasing contribution of the reflected radiation from the gas-dust torus. Our data show that there exists some anticorrelation between EWFeK\documentclass[12pt]{minimal}
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\begin{document}$L_{\mathrm{corr}}$\end{document}, but it is not strong. We have not found statistically significant deviations from the AGN Unified Model.
