Fig. 11.

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Left of the black vertical line: distribution of the median ∑SFR (top panel) and for the total SFR (bottom panel) for RDAGN galaxies (green) and their controls (brown). We calculate these quantities using all spaxels with a S/N > 0 in all emission-lines used for classification. Right of the black vertical line from left to right: distribution of the median ∑SFR (top panel) and for the total SFR (bottom panel) for RDAGN galaxies (green) and their controls (brown) for the entire sample, LTGs, and ETGs. These quantities are derived from spaxels with a S/N > 3. When no spaxels in the galaxy meet the relevant criteria, the median or total SFR is set to “NaN”.
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