Fig. 2.
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Histograms of the number of stars from the P1P2 sample (with masses M/M⊙ ≤ 1.2) with a probability > 99% of positive detection of solar-like oscillation in (1 LOP, BOL, δνenv = 0.5νmax) conditions. Top: distribution in Teff; middle in stellar mass; bottom: in stellar radius. The color code represents the assumed observing duration.
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