RXCJ2359.3-6042 shown in the DSS optical image overlaid with the XMM-Newton X-ray contours in the [0.5–2] keV band from the same data as in Fig. 2. The contours are obtained from a background subtracted image where the first contour traces 3 × 10-5 counts s-1 pix-1. The flux of the contours increases by steps of 1.5 subsequently. The compact component with high X-ray emission is centred at the galaxy at 23h59m04.2s in RA and –60d36m34s in Dec.
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