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Fig. 1

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Left panel top panel: original observed central spectrum (central spaxel) of IC 1256 (black line) and the one corrected from emission using GANDALF (red line). Bottom panel: emission line spectrum. Right panel top panel: fit to the central spectra of the galaxies from the sample (red line). Bottom panel: residuals from the fit. Masked areas are indicated with vertical lines.

This figure is made of several images, please see below:

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