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Fig. 9.
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Likelihood of the intrinsic Hα luminosities associated with the stellar population models presented in Sect. 4. The data points show the inferred Hα luminosity from Spitzer/IRAC data when it is either unattenuated (black) or attenuated relatively significantly with E(B − V) = 0.4 (i.e. AHα ≈ 1).
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