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Fig. 10


Ratio of Hα to UV-based SFRs (not corrected for dust extinction) as a function of Estar(BV) derived from the IRX ratio. The lines are the Eq. (7) with different values of f from Kashino et al. (2013) and Calzetti et al. (2000), as the legend indicates. The gray shaded area marks the confidence interval for our estimate of the f-factors.

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