$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3275f1.eps}\end{figure}$ Figure 1: Combined PN+MOS, background subtracted, 0.2-10 keV lightcurves of the four quasars. The time binning is 500 s for the radio-loud quasars and 1000 s for the radio-quiet quasars.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{aa3275f2.eps} \end{figure}$ Figure 2: Power law fit with free absorption for PKS 2149-306in the 0.2-8 keV energy range. The upper panel shows the PN fit, the middle panel the ratio between data and model; the lower panel gives for a comparison the ratios for the power law fit to the combined MOS1 plus MOS2 data.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3275f3.eps} \end{figure}$ Figure 3: Power law fit with galactic absorption for PKS 2126-158over the restricted energy band 2-10 keV, extrapolated to lower energies.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3275f4.eps} \end{figure}$ Figure 4: Power law fit with free absorption to the PN data for PKS 2126-158 (upper and middle panel). The lower panel shows the ratios between data and model for the warm absorber fit with galactic absorption to the PN data.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3275f1.eps}\end{figure}$	Figure 1: Combined PN+MOS, background subtracted, 0.2-10 keV lightcurves of the four quasars. The time binning is 500 s for the radio-loud quasars and 1000 s for the radio-quiet quasars.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{aa3275f2.eps} \end{figure}$	Figure 2: Power law fit with free absorption for PKS 2149-306in the 0.2-8 keV energy range. The upper panel shows the PN fit, the middle panel the ratio between data and model; the lower panel gives for a comparison the ratios for the power law fit to the combined MOS1 plus MOS2 data.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3275f3.eps} \end{figure}$	Figure 3: Power law fit with galactic absorption for PKS 2126-158over the restricted energy band 2-10 keV, extrapolated to lower energies.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3275f4.eps} \end{figure}$	Figure 4: Power law fit with free absorption to the PN data for PKS 2126-158 (upper and middle panel). The lower panel shows the ratios between data and model for the warm absorber fit with galactic absorption to the PN data.
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$\begin{figure} \par\psfig{figure=3275.f10,height=6.3truecm,width=8.8truecm,angle=-90,% bbllx=113pt,bblly=43pt,bburx=557pt,bbury=711pt,clip=} \end{figure}$	Figure 5: Combined PN+MOS power law fit with galactic absorption for Q 0000-263in the 0.2 - 9 keV energy range. The lower panel gives the $\Delta \chi ^2$ per channel.
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$\begin{figure} \psfig{figure=3275.f11,height=6.3truecm,width=8.8truecm,angle=-90,% bbllx=113pt,bblly=43pt,bburx=557pt,bbury=711pt,clip=}\end{figure}$	Figure 6: Combined PN+MOS power law fit with galactic absorption for Q 1442+2931in the 0.2 - 9 keV energy range. The lower panel gives the $\Delta \chi ^2$ per channel.
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