Fig. B.2.
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Five best cases of radial profiles of line ratios. Cyan (violet) dots mark the logarithm of [O III]λ5007/Hβ ([Ne III]λ3869/[O II]λ3727) ratio as a function of the radius expressed in pixels (pixel 0 is the centre of the galaxy). Different markers are used to discriminate between pixels above (squares) and below (circles) the central pixel 0 in the slit (see also Fig. 2b). The ID of each object and the redshift are specified in the top left corner of each plot.
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