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Fig. 6.
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Histograms in Teff (top), and mass (bottom) for MS stars with M/M⊙ ≤ 1.2 in the P1P2 sample assuming (1 LOP, BOL, 730 days, δνenv = νmax/2) conditions with expected detection of solar-like oscillations and satisfying cases IIa and IIIa listed in Table 6.
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