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Fig. 5


Radial distribution of the intensities for the [FeII] (blue stars), Brγ (green dots), and H2 (red squares) emission lines as derived from GANDALF. Displayed points each have an S/N > 3. The seeing disk (and nuclear aperture) is indicated with the black bar. The off-nuclear apertures are delimited by the vertical dashed lines at (+/−)375 pc and (+/−)125 pc. The minimum and maximum 1σ error for each emission line are displayed in the upper right corner.

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