Open Access
Table 1
Parameterization of the quadratic limb darkening in the Kepler band (as per Claret & Bloemen 2011) for the main-sequence stars shown in Fig. 3.
| Spectral type | Teff | a | b | oLD |
|---|---|---|---|---|
| A5 | 8500 | 0.2474 | 0.3026 | 0.153 |
| F5 | 6500 | 0.2987 | 0.3098 | 0.178 |
| G2 | 5750 | 0.4089 | 0.2556 | 0.218 |
| K5 | 4500 | 0.6809 | 0.0645 | 0.312 |
| M0 | 4000 | 0.5444 | 0.1898 | 0.271 |
Notes. All stars have log(g) = 4.5. The corresponding radius overshoot following from Eq. (3) is shown in the last column.
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