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Fig. 20

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Sub-DLA detected towards J223941.8-294955 at zabs = 1.825. The spectrum is smoothed with a boxcar average of 1.0 pixel for plotting reasons. The solid red line corresponds to the Voigt profile fit to the sub-DLA with an inferred column density of log NH   I = 19.84 ± 0.14. Emission is clearly seen in the trough of this absorber which is likely to correspond to the Lyman-α emission from the sub-DLA host.

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