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Table 1
The best-fit coefficients of the three effects and the occultation, using the Q2 and the Q3 data.
| Q2 | Q3 | |||
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| BEER model: | ||||
| Abeam | 8.6 ± 1.1 | 10.4 ± 1.0 | ppm | BEaming |
| Aellip | 66.8 ± 1.6 | 69.1 ± 1.5 | ppm | Ellipsoidal |
| Arefl | 72.0 ± 1.5 | 72.0 ± 1.4 | ppm | Reflection |
| a2s | −1.0 ± 1.0 | −3.3 ± 1.1 | ppm | – |
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| Primary transit: | ||||
| a/R∗ | 3.16 ± 0.08 | 3.17 ± 0.06 | Semi-major axis to stellar radius | |
| rp/R∗ | 0.0908 ± 0.0005 | 0.0907 ± 0.0005 | Planetary to stellar radii | |
| b | 0.75 ± 0.01 | 0.75 ± 0.01 | Impact parameter | |
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| Secondary occultation: | ||||
| depth | 163.8 ± 3.8 | 157.8 ± 3.5 | ppm | |
| Δφ | −0.0007 ± 0.0005 | −0.0012 ± 0.0005 | ||
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