Left figure: residuals (RSP − RLEG) between the radius of each of the 66 stars in the Kepler LEGACY sample delivered by SPInS (RSP) and the values RLEG obtained from full optimisations of stellar models based on their individual oscillation frequencies by different pipelines (see e.g. Silva Aguirre et al. 2017). Right figure: same comparisons for the mass. SPInS inference is based on observational constraints on Teff, [Fe/H], log g, ⟨Δν⟩, and νmax. The position of KIC 7771282, as modelled by the GOE pipeline is the pink diamond outlier at RSP ≈ 1.66 R⊙ (RLEG, GOE ≈ 1.4 R⊙) and MSP ≈ 1.3 M⊙ (MLEG, GOE ≈ 0.8 M⊙). Symbol colours and shapes identify the pipelines as explained in the legend.
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