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Fig. 11.

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Histograms showing the number of times each best model was returned from the three sets of 100 perturbed g-mode period spacing patterns derived from the LCSAP, LCPDC and LCPápics light curves. The parameters of the models are given in Table 4. Solutions based on a four-, five- and six-parameter setup are shown in the top, middle and bottom panels, respectively. The model names in red (i.e. 4A, 5C and 6A) are the best models determined by Michielsen et al. (2021) using the g-mode period spacing pattern from Pápics et al. (2015).

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