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Table 2.
Numbers of stars in the P1P2 sample in 1 LOP with expected detection of solar-like oscillations after 730 days of observation and assuming δνenv = νmax/2.
| Cases | BOL | EOL |
|---|---|---|
| All | 5858 | 5553 |
| MS stars | 2751 | 2449 |
| M < 1.6 | 4744 | 4439 |
| M < 1.6, MS stars | 2732 | 2430 |
| M ≤ 1.2 | 1245 | 1106 |
| M ≤ 1.2, MS stars | 1016 | 830 |
| R ≤ 1.1 | 269 | 203 |
Notes. Stellar masses, M, and radii R in solar units.
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