Fig. 6.
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|RM| as function of redshift for the spectroscopic sample. Upper panel: observed |RM| in rad m−2 vs. redshift for all 81 sources in the COSMOS field. The black line represents the best fit including all data points. Lower panel: observed |RM| in rad m−2 vs. redshift for all 44 sources in the XMM-LSS field. Again, the black line represents the best fit. For both fields all error bars show the 68% interval around |RM|.
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