Fig. A.1.
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Channel maps of the VLA detection in the rest frame of the source. Blue contours represent the data, with dark blue lines denoting positive emission and light dashed blue lines the negative. Contours are plotted starting from 3 times the noise in the cube (0.65 mJy beam−1), and are spaced by a factor of 2 in intensity. The black X indicates the H I centroid of the galaxy.
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