All Figures

$\begin{figure} \par\epsfig{file=ms3735_f1.ps,width=16cm} \end{figure}$ Figure 1: The contours of the X-ray emission in sigmas of significance. Lowest contour and stepwidth 1 sigma. The contours are overlaid over the SOFI/NTT image taken in the K-band. The squares indicate galaxies with J-K=2-2.4corresponding to early type galaxies with redshifts approximately beyond 1.0. The three spectroscopically confirmed members of EIS J0533-2412 are indicated by circles. The crosses show the center of the galaxy concentrations.
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In the text

$\begin{figure} \par\epsfig{file=ms3735_f2.eps,width=8.5cm} \end{figure}$ Figure 2: Zoom on EIS J0533-2412. The contours of the X-ray emission are overlaid over the VLT/FORS2 image taken in R-band. The exposure of the VLT-image is 10 min. Same symbols as in Fig. 1.
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In the text

$\begin{figure} \par\epsfig{file=ms3735_f3.eps,width=8.5cm} \end{figure}$ Figure 3: Surface brightness profile of XMMU J053344.4-241048. The profile is summed over MOS1 and MOS2. The error bars for the surface brightness are 1 $\sigma$ uncertainties. The full line corresponds to the point source model by Ghizzardi (2001) plus background. The dotted line is a beta-model convolved with the PSF of XMM-Newton with $\beta =2/3$ and $\Theta _{\rm c}=0.026'$ . This model is marginally consistent with the data (see text).
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In the text

$\begin{figure} \par\epsfig{file=ms3735_f4.eps,width=8.5cm} \end{figure}$ Figure 4: Surface brightness profile of XMMU J053337.8-241250. The profile is summed over MOS1 and MOS2. Error bars and full line are identical to Fig. 3. The dotted line is a beta-model convolved with the PSF of XMM-Newton with $\beta =2/3$ and $\Theta _{\rm c}=0.073'$ . This model is marginally consistent with the data (see text).
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In the text

$\begin{figure} \par\epsfig{file=ms3735_f2.eps,width=8.5cm} \end{figure}$	Figure 2: Zoom on EIS J0533-2412. The contours of the X-ray emission are overlaid over the VLT/FORS2 image taken in R-band. The exposure of the VLT-image is 10 min. Same symbols as in Fig. 1.
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$\begin{figure} \par\epsfig{file=ms3735_f4.eps,width=8.5cm} \end{figure}$	Figure 4: Surface brightness profile of XMMU J053337.8-241250. The profile is summed over MOS1 and MOS2. Error bars and full line are identical to Fig. 3. The dotted line is a beta-model convolved with the PSF of XMM-Newton with $\beta =2/3$ and $\Theta _{\rm c}=0.073'$ . This model is marginally consistent with the data (see text).
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