Open Access
Table C.1
Model parameters for the normalisation and the systematic noise. The values reported are the one obtained for the phase-curve model with a Lambertian reflector and a sinusoid approximation of the thermal emission. All parameters had uniform priors with the sole purpose of improving convergence speed of the MCMC run.
| Parameter | Symbol | Value | Units |
|---|---|---|---|
| Stellar flux used for normalisation |  |
147277.2 ± 3.5 | 103 e− |
 |
 |
103 e− | |
 |
 |
103 e− | |
 |
 |
103 e− | |
 |
146500 ± 20 | 103 e− | |
 |
146468 ± 20 | 103 e− | |
| Quadratic and linear trends |  |
 |
ppm∕day2 |
 |
−631 ± 39 | ppm∕day | |
 |
2005 ± 173 | ppm∕day2 | |
 |
 |
ppm∕day | |
 |
 |
ppm∕day2 | |
 |
−95 ± 30 | ppm∕day | |
 |
 |
ppm∕day2 | |
 |
 |
ppm∕day | |
 |
 |
ppm∕day | |
 |
 |
ppm∕day | |
| Roll angle coefficients for the eclipses | a1, ecl | 28 ± 10 | ppm |
| b1, ecl | 92 ± 43 | ppm | |
| a2, ecl |  |
ppm | |
| b2, ecl | −24 ± 16 | ppm | |
| a3, ecl | −16 ± 16 | ppm | |
| b3, ecl | −30 ± 21 | ppm | |
| a4, ecl | −13 ± 11 | ppm | |
| b4, ecl | 4 ± 11 | ppm | |
| a5, ecl |  |
ppm | |
| b5, ecl |  |
ppm | |
| Roll angle coefficients for the phase curves | a1, PC |  |
ppm |
| b1, PC |  |
ppm | |
| a2, PC |  |
ppm | |
| b2, PC |  |
ppm | |
| a3, PC |  |
ppm | |
| b3, PC | −21 ± 101 | ppm | |
| a4, PC | 30 ± 42 | ppm | |
| b4, PC |  |
ppm | |
| a5, PC | 6.8 ± 8.2 | ppm | |
| b5, PC | 17 ± 11 | ppm | |
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