Table 5
Estimated uncertainties on the inverted rotation coefficients for the 15 stars of different types in our sample (left) and 1000 stars (right) for only ℓ = 1 modes, with the standard 10 radial orders centred about νmax.
| Stellar | N stars |
|
σ(ΔΩ) | N stars |
|
σ(ΔΩ) |
| type | [nHz] | [nHz] | [nHz] | [nHz] | ||
|
|
||||||
| F | 5 | 226 | 527 | 600 | 20 | 48 |
| G | 7 | 245 | 398 | 350 | 34 | 56 |
| K | 3 | 327 | 488 | 50 | 80 | 119 |
Notes. Instead of listing the uncertainty for each type of stellar model, 
, we list the mean of the uncertainties, .
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