Fig. C.1.
Lyα emission and the observed H I Lyman series line with the larger S/N in the velocity space for 15 of the 22 galaxies in our sample. The Lyα flux has been smoothed to the resolution of the Lyman series and scaled down by an arbitrary power law for display purpose. Gray-shaded regions show contamination from the geocoronal emission or Milky Way absorption lines next to the H I absorption line.
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