Fig. H.1.
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Top panel: Simulated power spectral density (PSD) for RGB star. Middle panel: Observed PSD, divided by granulation background. Bottom panel: Simulated PSD for a late-clump/early AGB star. For the simulated PSD, the mixed ℓ = 1 modes are highlighted, with an amplitude proxy calculated from the mode inertia and a Gaussian envelope.
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