Fig. C.1.

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Spectra of the VLA BC-configuration BCD detections at a velocity resolution of 5 km s−1. The horizontal line over-plotted below each spectrum indicates the W20 velocity range. The black vertical lines on the W20 line are the VHI calculated, using the Vsysw20 method from (Reynolds et al. 2021). VHI (Vsysw20 method) and W20 measurements for each galaxy in this figure are shown in Table 2.
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