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Fig. 9


Comparison between star formation rates derived from the SED fitting (SFRSED), the extinction-corrected Hα luminosity (SFRHα), and the rest-frame attenuation-corrected FUV luminosity (SFRFUV) for the sample of EELGs. The solid lines indicate the one-to-one relation.

This figure is made of several images, please see below:

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