Fig. 5.

Best-fit line model fit to C IV λλ1548, 1551 detected with MUSE. The green and orange dashed lines represent the underlying doublet emission at wavelengths of 1548 Å and 1551 Å, which are the rest-frame velocities, in the upper and lower axes, respectively. Three Voigt profiles model the absorbers for each emission line in the doublet.
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