Table 6
Estimated uncertainties weighted by the distribution of expected inclinations on the inverted rotation coefficients.
| Stellar | N stars |
|
σ(ΔΩ) | N stars |
|
σ(ΔΩ) |
| type | [nHz] | [nHz] | [nHz] | [nHz] | ||
|
|
||||||
| F | 5 | 232 | 628 | 600 | 21 | 57 |
| G | 7 | 262 | 508 | 350 | 37 | 71 |
| K | 3 | 357 | 489 | 50 | 87 | 119 |
|
|
||||||
| F | 5 | 90 | 273 | 600 | 8 | 24 |
| G | 7 | 72 | 140 | 350 | 10 | 19 |
| K | 3 | 88 | 133 | 50 | 21 | 32 |
Notes. Stars of each main-sequence type in our sample of stellar models (left) and 1000 stars (right). Using only ℓ = 1 modes in the top half and ℓ = 1,2 modes in the lower half of the table with the standard 10 radial orders centred about νmax.
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