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Fig. 8.
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fνmax as a function of metallicity for Kepler red giants (Li et al. 2024a), the low metallicity red-giants KIC 8144907 (Huber et al. 2024), KIC 7693833 and KIC 4671239 (Larsen et al. 2025), and HD 175305 and HD 128279 (Lindsay et al. 2025), as well as the subgiants ν Indi (Chaplin et al. 2020) and HD 140283.
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