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Fig. 9.
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RRM rms (left) and ⟨p⟩ (right) of the LoTSS RRM sample with a GRM limit of 14 rad m−2 versus LOS projected separation in virial radii from galaxies of the three samples of stellar mass M* > 1011 M⊙, M* = 1010–1011 M⊙, and M* = 109–1010 M⊙. The bin size is of 0.15 virial radii.
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