$\begin{figure} \par\includegraphics[width=6cm,clip]{8319fig8.ps}\end{figure}$ Figure 2: Reflection fraction versus photon index in our sample. Dot-dash box shows the average values found in the Beppo-SAX sample of type 2 AGN (Risaliti 2002).
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In the text

$\begin{figure} \par\mbox{\includegraphics[origin=rb,angle=-90,width=5.8cm,clip]{... ...ludegraphics[origin=rb,angle=-90,width=5.8cm,clip]{8319fig12.ps} }\end{figure}$ Figure 3: The iron line profile when the continuum is reproduced with model C. For NGC 788 stars, triangles, circles and squares represents SIS0, SIS1, GIS2, and GIS3 respectively For IC 4518A, ESO 103-G35, and IGR J10404-4625 triangles, circles, and squares represent MOS1, MOS2, and pn data respectively.
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{8319fig17.ps}\end{figure}$ Figure 5: Absorbing column density versus Fe equivalent width. The dotted line represent the best fit constant in the region $N_{\rm H}<3\times 10^{23}$ cm^-2. The box regions represent the average values of $N_{\rm H}$ (1 $\sigma$ errors) found in the Beppo-SAX sample of type 2 AGN (Risaliti 2002).
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7cm,clip]{8319fig1.ps}\hspac... ...cs[angle=-90,width=7cm,clip]{8319fig7.ps}\hspace{4mm}\hspace{7cm} \end{figure}$	Figure 1: Spectra and data/model ratio for all sources of our sample. The ratios are plotted using our model A: absorbed power-law+thermal emission+iron line.
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$\begin{figure} \par\includegraphics[width=6cm,clip]{8319fig8.ps}\end{figure}$	Figure 2: Reflection fraction versus photon index in our sample. Dot-dash box shows the average values found in the Beppo-SAX sample of type 2 AGN (Risaliti 2002).
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$\begin{figure} \par\mbox{\includegraphics[origin=rb,angle=-90,width=5.8cm,clip]{... ...ludegraphics[origin=rb,angle=-90,width=5.8cm,clip]{8319fig12.ps} }\end{figure}$	Figure 3: The iron line profile when the continuum is reproduced with model C. For NGC 788 stars, triangles, circles and squares represents SIS0, SIS1, GIS2, and GIS3 respectively For IC 4518A, ESO 103-G35, and IGR J10404-4625 triangles, circles, and squares represent MOS1, MOS2, and pn data respectively.
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$\begin{figure} \mbox{\includegraphics[origin=rb,angle=-90,width=5.8cm,clip]{8319... ...ludegraphics[origin=rb,angle=-90,width=5.8cm,clip]{8319fig16.ps} }\end{figure}$	Figure 4: Contour plots 99, 90, 68 percent of the intrinsic width $\sigma$ vs. Energy for the iron lines.
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$\begin{figure} \par\includegraphics[width=6cm,clip]{8319fig17.ps}\end{figure}$	Figure 5: Absorbing column density versus Fe equivalent width. The dotted line represent the best fit constant in the region $N_{\rm H}<3\times 10^{23}$ cm^-2. The box regions represent the average values of $N_{\rm H}$ (1 $\sigma$ errors) found in the Beppo-SAX sample of type 2 AGN (Risaliti 2002).
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$\begin{figure} \par\includegraphics[width=6cm,clip]{8319fig18.ps}\end{figure}$	Figure 6: High energy cutoff in keV versus photon index.
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