Fig. 1.
Top left: g − r − i image composite from SDSS for MaNGA galaxy 8150−6103, with the MaNGA IFU hexagonal FoV overlaid. East is to the left. Top right: example of our fitting procedure for the [S III] lines for one representative spaxel in this example galaxy. The black solid line is the observed spectrum, while the dashed-dotted red line is the best fit. The regions in grey were masked before fitting. Bottom panels: [S III]λ9532 flux, velocity, and velocity dispersion maps of MaNGA galaxy 8150−6103.
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