The nature of LOFAR rotation measures and new constraints on magnetic fields in cosmic filaments and on magnetogenesis scenarios

Open Access

Fig. 1.

RRM rms as a function of the GRM limit and Galactic latitude. Left: RRM rms of the spectroscopic redshift sample filtered by different GRM limits. The orange circle highlights the case with a limit of 14 rad m⁻². Right: RRM rms as a function of Galactic latitude |b| for the case filtered with GRM_th = 14 rad m⁻².

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