Fig. 5.
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RRM rms (top left), distribution (top right), and mean fractional polarisation (bottom left) of the full spectroscopic sample at 144 MHz in bins of the separation from the nearest galaxy cluster of mass M > 1.0 × 1014 M⊙ along the LOS. Bottom right: Same as the for the top left panel except it is for galaxy clusters of mass M < 1.0 × 1014 M⊙.
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