Fig. 5.
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Kernel density estimators for the ratio of radii derived from SBCR and asteroseismology, using the Pietrzyński et al. (2019) SBCR. The solid blue and red lines represent the results for RGB and RC stars, respectively, based on the Yu et al. (2018) dataset. The dashed lines correspond to the results obtained using the APO-K2 dataset.
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