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Table 2
Extrapolated values of R* and M* using Teff from polynomials derived from interferometric measurements of M and K dwarf stars (Eqs. (8) and (10), Boyajian et al. 2012), for the three simulated host stars combined with the calculated log g and u1 and u2 for the quadratic limb darkening law from Claret (2017).
| Spectral | Teff | R* | M* | logg | u1 | u2 |
|---|---|---|---|---|---|---|
| type | (K) | (R⊙) | (M⊙) | (cgs) | ||
| M4V | 3200 | 0.155 | 0.10 | 5.06 | 0.1533 | 0.4776 |
| M1V | 3700 | 0.493 | 0.52 | 4.77 | 0.1737 | 0.4118 |
| K5V | 4100 | 0.623 | 0.65 | 4.66 | 0.3955 | 0.2618 |
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