Fig. A.8

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MCXC J0056.0-3732, a case in which the RXGCC position has an offset with respect to the X-ray peak due to a nearby point source. We have associated the MCXC and RXGCC clusters because both detections come from the same X-ray emission, although the RXGCC catalogue has chosen an incorrect redshift (from the nearby cluster Abell S 102) and its flux may be contaminated. The left and right panels show the RASS and XMM-Newton images, respectively. The positions of MCXC J0056.0-3732 (z = 0.163) and RXGCC 42 (z = 0.056) are marked with a light blue cross and a small red circle, respectively. The corresponding solid and dashed circles represent the size θ500 of the clusters and their aperture radius. The magenta plus represents the position of Abell cluster Abell S 102 (z = 0.056).
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