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Fig. C.1.

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Average W80 binned on a plane of M vs. L[O III]. The bins have a size of 0.3 dex in each parameter, colored by the strength of the W80. The scatter dots show the distribution of a specific galaxy population and the line shows a 1D polynomial fitted to the location of the SF galaxies. The green arrows in the plots illustrate the gradient change of W80 in the parameter space, with the arrowhead indicating the direction and the arrow’s size representing the magnitude.

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