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Fig. 7


Emission-line profiles and component decomposition for the Hα  and [N ii](λ6548, 6584)  complex. Upper panel: spectrum extracted for the central component (radius of 0.̋9 or 3.4 kpc around the galaxy center) of the host galaxy from the MUSE data cube; lower panel: X-shooter spectrum. The contribution from [N ii] is shown in red; the total sum of the emission-line model in black. For Hα, we also plot the three individual Gaussian components with dashed lines.

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