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Fig. 1

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eROSITA X-ray image of A3667 in the soft X-ray band with radio contours (170–231 MHz) from the GaLactic and Extragalactic All-Sky MWA Survey (Wayth et al. 2015). The well-known radio relics and the substructure in the northwest are clearly visible. The image was created and corrected using the methods described in Sect. 2.1. The color bar is in units of counts per second (as in all following images). In addition, the characteristic radii R500 and R200 are displayed.

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