Table 1: Coordinates of the AGN and the cluster. The AGN is almost at the centre of the cluster emission. We also show the count rate for the two objects (normalized for the different apertures, see text for details) and the luminosities, both in the [0.3-10 keV] band (bolometric luminosity for the cluster is given in Table 2). The contribution of the AGN is larger than the cluster luminosity. Both objects are at the same redshift of 0.52. An optical counterpart of the AGN is marked in Fig. 7.
Name $\alpha_{2000}$ $\delta_{2000}$ Counts [cts/s] $L_{\rm X}$ [erg/s]

AGN 03 01 07.8 -47 06 24.0 0.07 $1.8\times 10^{44}$

RBS 380 03 01 07.6 -47 06 35.0 0.05 $1.6\times 10^{44}$

**Table 1:** Coordinates of the AGN and the cluster. The AGN is almost at the centre of the cluster emission. We also show the count rate for the two objects (normalized for the different apertures, see text for details) and the luminosities, both in the [0.3-10 keV] band (bolometric luminosity for the cluster is given in Table 2). The contribution of the AGN is larger than the cluster luminosity. Both objects are at the same redshift of 0.52. An optical counterpart of the AGN is marked in Fig. 7.
Name	$\alpha_{2000}$	$\delta_{2000}$	Counts [cts/s]	$L_{\rm X}$ [erg/s]
AGN	03 01 07.8	-47 06 24.0	0.07	$1.8\times 10^{44}$
RBS 380	03 01 07.6	-47 06 35.0	0.05	$1.6\times 10^{44}$

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