All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{9599f1.ps}\end{figure}$ Figure 1: Wavelet-decomposed 0.5-2.0 keV image of Abell 222 (to the South) and Abell 223 (the two X-ray peaks to the North). We show only sources with >5 $\sigma$ detection, but for these sources we follow the emission down to 3 $\sigma$ . The filament connecting the two massive clusters is clearly visible in the image. The regions used to extract the filament spectrum and to determine the background parameters are indicated by red and yellow circles, respectively.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.8cm,clip]{9599f2.ps}\end{figure}$ Figure 2: The spectrum of the filament between the clusters A 222/223 - the data points on the top were obtained by EPIC/pn and below by EPIC/MOS. The contributions from the X-ray background and from the filament to the total model are shown separately.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.8cm,clip]{9599f2.ps}\end{figure}$	Figure 2: The spectrum of the filament between the clusters A 222/223 - the data points on the top were obtained by EPIC/pn and below by EPIC/MOS. The contributions from the X-ray background and from the filament to the total model are shown separately.
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