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Fig. 3.
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Histograms of the number of stars (MS stars with M < 1.6 M⊙ and subgiants) from the P5 sample with an expected detection of solar-like oscillations with at least 99% probability assuming 730, 365, 90, and 30 days of observations. Conditions are (1 LOP, BOL, δνenv = 0.5νmax).
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