Fig. 7.
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Two slices through the 24″ tapered H I cube made for a typical MeerKAT 5 h observation. These slices show no artefacts due to residual RFI or continuum subtraction errors. Typically, the RA-velocity slices show some faint vertical structure in channel ranges that are excluded from the visibility spectral fit described in Sect. 3.5 (in this case, ∼1200–∼1500 km s−1).
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