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Fig. 4

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Comparison of the global asteroseismic parameters measured by our algorithm to those reported in the literature. Stars are coloured by the number of modules in which they produce a flag; pink for a single module, brown for two modules, and an open grey marker for none. Triangles represent stars for which no uncertainty on vmax was reported in the literature. Targets λ2 For, v Ind, and HD 212771, which are discussed in the text, are marked with a diamond, circle, and square, respectively. The left and right panels show the fractional difference between the values of vmax and ∆v as measured by the algorithm vs literature value, respectively.

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