Aims. The radio halo in the Coma cluster is unique in that its spectrum has been measured over almost two decades in frequency. The current radio data show a steepening of the spectrum at higher frequencies, which has implications for models of the radio halo origin. There is an on-going debate on the possibility that the observed steepening of the spectrum and the apparent shrinking of the halo-size at higher frequencies is not intrinsic to the emitted radiation, but is instead caused by the Sunyaev-Zeldovich (SZ) effect.
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