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Fig. 4.

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Excess |RM| as function of impact parameter for the spectroscopic samples. Upper panel: observed |RM| in rad m−2 vs. impact parameter in kpc for all 81 sources in the COSMOS field. The green bar indicates a bin of individual data points with the blue line being the error bar. The data points are color-coded with respect to the star-formation rate of each galaxy. Lower panel: observed |RM| in rad m−2 vs. impact parameter in kpc for all 44 sources in the XMM-LSS field. Here, the data points are color-coded with respect to the u-band magnitude of each galaxy. For both fields all error bars show the 68% interval around |RM|.

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