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Table 7
Input parameters for the ellipsoidal and reflection modulations fitting.
| Fixed parameters (input) | |||
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| Parameter | Value | Explanation | Origin |
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| T eff | 4550 ± 75 K | Effective temperature | Spectroscopy (Sect. 3.4) |
| log g | 2.953 ± 0.007 | Surface gravity | Asteroseismology (Sect. 3.5.1) |
| [Fe/H] | 0.11 ± 0.07 | Stellar metallicity | Spectroscopy (Sect. 3.4) |
| P | 6.246580 ± 0.000082 days | Orbital period | Light curve (Batalha et al. 2013) |
| Ω | 0° | Longitude of the ascending node | Assumed |
|
575 nm | Effective wavelength of the Kepler band | |
| M ∗ | 1.31 ± 0.10 M⊙ | Stellar mass | Asteroseismology (Sect. 3.5.3) |
| R ∗ | 6.30 ± 0.16 R⊙ | Stellar radius | Asteroseismology (Sect. 3.5.3) |
| Rp/R∗ |
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Planet-to-star radius | Transit fitting (Sect. 4.1) |
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| Free parameters (output) | |||
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| Parameter | [Lower limit , Upper limit] | Explanation | |
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| e | [0.0,0.5] | Eccentricity | |
| ω | [0°,360°] | Argument of periastron | |
| M p | [0.5 MJup,6.0 MJup] | Planet-to-star mass ratio | |
| a/R⋆ | [1.5,5.0] | Semi-major axis to stellar radius ratio | |
| i | [60°,90°] | Orbital inclination | |
| Φoffset | [−0.05,0.05] | Phase offset in phase units | |
Notes.We list the fixed values and the value ranges used by the genetic algorithm to compute the final solution.
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