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Fig. B.1.

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Extraction of the wind component from the Hα line in four galaxies of the DWALIN-19 sample. The individual panels are analogous to those shown in Fig. 6, with the galaxy name indicated on top of panel (a). To improve their visualisation, the intensity maps have been smoothed to a resolution (FWHM) of ∼1.5″. Iso-intensity contours in panels (e1) and (e2) are spaced by a factor of three, with the outermost being at an intensity level indicated in the bottom-left corner of panel (e1) (in units of erg s−1 cm−2, corresponding to 4σnoise), both for the whole emission (grey contours) and for the wind component alone (black contours). No contours are shown when fluxes are below such value.

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