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Fig. 5


Shape measurement for HI line profiles. The figure shows the ALFALFA spectrum for the galaxy with the lowest (top panel) and highest (bottom panel) kurtosis in the α.btfr sample. The parts of the spectrum that have been used for measuring the kurtosis are highlighted with a thick red line. Profile kurtosis is a measure of the peakiness of the profile, and so the top and bottom panels respectively represent the most double-horned and the most peaked profiles among the α.btfr galaxies.

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