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Fig. 8.
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RRM rms (top left) and ⟨p⟩ (top right) of the LoTSS RRM sample with a GRM limit of 14 rad m−2 versus source separation in kiloparsecs from galaxies of stellar mass M* > 1011 M⊙. The bin size is of 50 kpc. Bottom: as for top panels, except the separation is in virial radii, with bin size of 0.15 virial radii.
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