Fig. 18.

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Maps of the for three example galaxies at the individual spaxel level. We show in blue contours the Hα surface brightness and in red the regions masked as foreground stars. The
maps demonstrate the quality of our spectral fits
, except in a few regions of bright Hα emission (e.g., the central regions in NGC 1672 and NGC 4535). A few regions of higher
can also be seen in the middle of spiral arms, corresponding to the centres of bright H II regions. Foreground stars appear as small spots of very high
and are emphasised with red contours.
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