Fig. 7.
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Long-slit spectra binned at 160 and 400 Å (thin and thick lines, respectively) obtained with the GMOS spectrographs at the Gemini North (top panel) and South (lower panel) Observatories. The vertical solid lines denote the position of Ly-α of its ‘mother’ QSO, the vertical dashed line the position of Ly-α based on the Le PHARE fits. The dwarf templates are at arbitrary normalizations.
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