Fig. 7.
Best fit line model to the intercombination Si IV λλ1393, 1402 + O IV] line detected with MUSE. The green and orange dashed lines represent the underlying doublet emission at the rest-frame wavelengths, 1393 Å and 1402 Å, which are fixed to the systemic velocity in the upper and low axes, respectively. The O IV] quintuplet line emission is shown in purple.
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