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Fig. 3.

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Diagnostic diagrams by Baldwin et al. (1981) (top row) and Veilleux & Osterbrock (1987) (bottom row) with emission line flux ratios extracted from the total emission line fluxes of the individual spaxels. The lime green icons indicate the base spectra for star formation (square), AGN emission (circle), and LINER emission (triangle). Our data points shown here are color-coded using the fraction of Hα emission that is ascribable to SF (left), AGN emission (middle), and LINER emission (right). The data points are smoothed over via LOESS (Cappellari et al. 2013).

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