Fig. 2.

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HI detection along the LOS to Nube. We also show different polarisations of the data, i.e. XX and YY, in order to better identify which other HI emission peaks in the spectrum are potentially spurious. The black tick indicates the location of the peak with the strongest signal in our data. We note that other distinct peaks are not always present in the two different polarisations, which reduces their relevance as real signals.

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