Fig. F.2.

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Spectra extracted from the 64 spatial bins (see Sect. 3.3) and Gaussian+Voigt fitting results. In each panel, the thick dark magenta line indicates the best fit model. The dot-dash red line and dashed blue line denote the narrow and broad emission components, respectively. The dotted olive lines are the summation of the two emissions. The calculated from each fit is shown as an indicator of the fit quality. We note that each spectrum is summed from the spatial bin, each of which contains a different number of spaxels. Hence, the fluxes of the spectra shown here are not to be compared directly.
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