Fig. 6
Measured FD from the Faraday cube at 90 cm versus RM values measured by Han et al. (1998) and Taylor et al. (2009) at 20 cm. The grey area marks the range of FD that probably is affected by foreground emission and instrumental polarization. Dashed lines indicate the expected rotation measure of the Galactic foreground, dotted lines show the range spanned by the FWHM of the RMSF.
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