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Fig. 5

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Results of ν sin i inferences. Left panel: positions of the sample stars in the spectroscopic HR diagram. Individual objects are colour coded according to their ν sin i value inferred from the Fourier method. Right panel: comparison of ν sin iSP with ν sin iFT. The grey line shows the case where ν sin iFT and ν sin iSP are equal, while the blue line is an error-weighted fit to the observed values.

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