Fig. 6.
Best-fit line model to N V λλ1238, 1242 detected with MUSE. The green and orange dashed lines represent the underlying doublet emission at the rest-frame wavelengths 1238 Å and 1242 Å, which are fixed to the systemic velocity in the upper and lower axes, respectively. Three Voigt profiles model the absorbers for each emission line in the doublet.
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