Fig. 9.
Distribution of galaxy clusters in the P1400 − M500 plane (adapted from Cassano et al. 2013, see it for details of the legend). MACS J1149 (red dot) has M500 = (10.4 ± 0.5)×1014 M⊙ and P1400 = (3.1 ± 0.9)×1024 W Hz−1; it is under-luminous with respect to the correlation by a factor of ∼3 and is located among the steep spectrum radio halos (green dots).
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