Fig. 2

Azimuthally averaged brightness profile of the radio emission in RXCJ1347 at 614 MHz. The profile is calculated in concentric annuli, as shown in the inset panel. The horizontal dashed-dotted line indicates the 3σ614 MHz noise level of the radio image. In our analysis we considered all data points above the 3σ614 MHz noise level. The black line indicates the best-fit profile described by an exponential law (dashed line, Eq. (3)) representing the mini-halo emission, and by a central Gaussian profile (dotted line, Eq. (2)) representing the central point source.
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