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Fig. 6.

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Models on the Teff − M* plane of the coarse grid. We show the goodness of the fit of each grid-point with no restrictions on the degree of the observed pulsation modes. The model with the lowest σrms is denoted with a white open circle, while the spectroscopic solutions are marked with black dots. The parameter space further investigated by a higher resolution sub-grid is indicated by a black square.

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