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Fig. 13

image

Increase of the spread of EVPA differences between 353 and 217 GHz as a function of offset angle between HI structures from integration in LVC and IVC ranges (‘Implementation 1’). All sky pixels with Nc > 1.5 are binned according to their Δ(θIVC, θLVC) values and the statistic is computed for each subsample with observational uncertainties propagated. The error bars in each bin represent the 1σ value of from a bootstrap resampling of the data 103 times per bin.

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