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Fig. 3
Models of uncertainties for the synthetic rotational splittings used for KIC 7341231 for the different modes, ℓ = 1,2 for 9 months of Kepler data from Appourchaux et al. (2012). The solid curves are a quadratic fit for each ℓ = 1,2 which we use to model the noise for the synthetic rotational splittings.
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