All Figures

$\begin{figure} \par\includegraphics[width=7.9cm,clip]{1775fig1.eps} \end{figure}$ Figure 1: The distribution in redshift and bolometric luminosity of Seyfert 1 type AGN observed with the high-resolution spectrometers on XMM-Newton and Chandra: filled shapes indicate that the presence of a warm absorber has been reported.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1775fig2.eps} \end{figure}$ Figure 2: Log $\xi$ $_{\rm avg}$ versus log $L_{\rm bol}$ for the objects in Table 3.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{1775fig3.eps} \end{figure}$ Figure 3: Log $N_{\rm Htot}$ versus log $L_{\rm bol}$ for the objects in Table 3.
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In the text

$\begin{figure} \par\includegraphics[width=8.1cm,clip]{1775fig4.eps} \end{figure}$ Figure 4: Average outflow velocity versus log $L_{\rm bol}$ for the objects in Table 3, excluding PG 0844+349 and PG 1211+143.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1775fig5.eps} \end{figure}$ Figure 5: Average outflow velocity versus log $N_{\rm Htot}$ for the objects in Table 3, excluding PG 0844+349 and PG 1211+143.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{1775fig6.eps} \end{figure}$ Figure 6: Average outflow velocity versus log $\xi$ $_{\rm avg}$ for the objects in Table 3, excluding PG 0844+349 and PG 1211+143.
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In the text

$\begin{figure} \par\includegraphics[width=8.1cm,clip]{1775fig7.eps} \end{figure}$ Figure 7: Total mass outflow rate of each AGN warm absorber ${\dot M}_{\rm out,total}$ plotted against ${\dot M}_{\rm acc}$ , the mass accretion rate of the AGN in each case. The line where ${\dot M}_{\rm out,total}={\dot M}_{\rm acc}$ is plotted for comparison.
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In the text

$\begin{figure} \par\includegraphics[width=14cm,clip]{1775fig8.eps} \end{figure}$ Figure 8: The estimated minimum ( $R_{\rm min}$ ) and maximum ( $R_{\rm max}$ ) distances of the warm absorber phases from the central engine as a ratio to the torus distance $R_{\rm torus}$ , plotted for each outflowing warm absorber phase in Table 5, in the order in which they appear in the table. The ratio of the BLR distance ( $R_{\rm BLR}$ ) to the torus distance is also plotted.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{1775fig9.eps} \end{figure}$ Figure 9: Log $v_{\rm avg}$ (Table 3) versus $\alpha _{\rm ox}$ (Table 4) for the AGN with outflowing warm absorbers.
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In the text

$\begin{figure} \par\includegraphics[width=7.9cm,clip]{1775fig1.eps} \end{figure}$	Figure 1: The distribution in redshift and bolometric luminosity of Seyfert 1 type AGN observed with the high-resolution spectrometers on XMM-Newton and Chandra: filled shapes indicate that the presence of a warm absorber has been reported.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{1775fig2.eps} \end{figure}$	Figure 2: Log $\xi$ $_{\rm avg}$ versus log $L_{\rm bol}$ for the objects in Table 3.
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$\begin{figure} \par\includegraphics[width=8.2cm,clip]{1775fig3.eps} \end{figure}$	Figure 3: Log $N_{\rm Htot}$ versus log $L_{\rm bol}$ for the objects in Table 3.
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$\begin{figure} \par\includegraphics[width=8.1cm,clip]{1775fig4.eps} \end{figure}$	Figure 4: Average outflow velocity versus log $L_{\rm bol}$ for the objects in Table 3, excluding PG 0844+349 and PG 1211+143.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{1775fig5.eps} \end{figure}$	Figure 5: Average outflow velocity versus log $N_{\rm Htot}$ for the objects in Table 3, excluding PG 0844+349 and PG 1211+143.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{1775fig6.eps} \end{figure}$	Figure 6: Average outflow velocity versus log $\xi$ $_{\rm avg}$ for the objects in Table 3, excluding PG 0844+349 and PG 1211+143.
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$\begin{figure} \par\includegraphics[width=8.1cm,clip]{1775fig7.eps} \end{figure}$	Figure 7: Total mass outflow rate of each AGN warm absorber ${\dot M}_{\rm out,total}$ plotted against ${\dot M}_{\rm acc}$ , the mass accretion rate of the AGN in each case. The line where ${\dot M}_{\rm out,total}={\dot M}_{\rm acc}$ is plotted for comparison.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=14cm,clip]{1775fig8.eps} \end{figure}$	Figure 8: The estimated minimum ( $R_{\rm min}$ ) and maximum ( $R_{\rm max}$ ) distances of the warm absorber phases from the central engine as a ratio to the torus distance $R_{\rm torus}$ , plotted for each outflowing warm absorber phase in Table 5, in the order in which they appear in the table. The ratio of the BLR distance ( $R_{\rm BLR}$ ) to the torus distance is also plotted.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{1775fig9.eps} \end{figure}$	Figure 9: Log $v_{\rm avg}$ (Table 3) versus $\alpha _{\rm ox}$ (Table 4) for the AGN with outflowing warm absorbers.
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