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Fig. B.1
Theoretical and observed power spectra of Kepler stars with similar masses (from top to bottom: 1.44, 1.48, 1.47 M⊙), Δν, and νmax. The heights in theoretical power spectra are in (m/s)2/μHz. The heights for observed spectra are given in ppm2/μHz divided by a factor 6000 to have scales similar to the theoretical spectra.
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