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Fig. 3.

image

Best-fitting Π0 values of our Π0-based asteroseismic modelling, based on three different grid setups (full, spectroscopic, and dynamical). Left panel: results of using a merit function and right panel: results of using an MD merit function. The vertical dashed black line represents the zero-point of the difference between the observational and theoretical Π0 (i.e. Π0, obs − Π0, theo = 0). The error bars are based on 68% HPD intervals of the Monte-Carlo parameter distributions.

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