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Fig. A.1.

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Band ratio F770W/F2100W grows with the Hα luminosity of the H II regions. This effect is seen for both observed (panel a) and stellar continuum subtracted (panel b) data in F770W. Panels c and d show the same line ratios after local background subtraction. The color denotes the number density of the regions, and the cyan curve represents a smoothed running median across the Hα luminosities.

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