Fig. 3.
Left panel: temperature distribution along the merging axis of CIZA2242. Right panel: abundance distribution along the merging axis of CIZA2242. The shaded areas represent the systematic uncertainties: green and orange shadows correspond to the background normalisation variation, and the blue one to the temperature structure. The shaded grey area shows the radio relic position. The dashed line shows the outer edge of the core spectral extraction region. The numbers and the BCGN blue point correspond to the regions and the red circle centred on BCGN, respectively, shown in Fig. 2.
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