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Fig. 2.

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Hα region of the spectra in two different regions of the galaxy. The left panel represent the approaching side of the galaxy, and the right panel shows the receding side. In both panels we show in blue the spectrum extracted from the science exposure after our updated sky subtraction procedure, in orange the sky spectrum associated with the exposure, while the grey dashed lines represent the expected position of Hα at v = 0 km/s.

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