Table 6.
Number of MS dwarfs with M ≤ 1.2 M⊙ stars in the P1P2 sample with expected positive seismic detection and satisfying different cases of MRA uncertainties.
| Case | BOL | EOL |
|---|---|---|
| Ia | 1016 | 880 |
| IIa | 1016 | 880 |
| IIIa | 260 | 195 |
| Ib | 1016 | 880 |
| IIb | 729 | 599 |
| IIIb | 206 | 146 |
Notes. Assumed conditions are (1 LOP, BOL, 730 days, δνenv = νmax/2). Labels a) and b) refer to frequency uncertainties assumed without and with a +0.5 shift due to the scatter in the fitted relation between δνℓ = 1, max and σLibb, ℓ = 1, max (Eq. (D.3)).
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