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Fig. 1.

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Histograms of the number of stars from the P1P2 sample (subgiants of all masses and MS stars with masses M/M < 1.6) with a probability of > 99% of positive detection of solar-like oscillation in the case of (1 LOP, BOL, νenv = 0.5νmax). Top: distribution in Teff, middle in stellar mass, bottom in stellar radius. The color code represents the assumed observing duration.

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