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Fig. 7

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Top: correlation between the SFR used in this work (from Hα) and those adopted by Huan et al. (2012) (computed from SED fitting) The one-to-one relation is given with a dotted line. Some outliers marked with their VCC names are commented on in the text. Bottom: the distribution of the residual of the two star formation indicators, with a Gaussian of mean μ and σ fitted to it.

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