Table D.1
Light-curve fitting parameters
| Parameter | Unit | Prior / Value | Application |
|---|---|---|---|
| Astrophysical model | |||
| Rp | RJ | N (0.148,0.0152) | all |
| t0 | d | U (59770.81,59770.86) | white |
| i | deg | N (87.83,0.252) | white |
| a | R* | N (11.4,12) | white |
| P | d | 4.0552765 | fixed |
| e | — | 0 | fixed |
| ω | — | 90 | fixed |
| Systematics model | |||
| c0 | — | N (1,0.052) | all |
| c1 | — | N (0,0.012) | all |
| c2 | — | N (0,0.012) | all |
Notes. For the application of our combined model parameters, ‘all’ refers to the parameter being free in both the fitting routines for the spectroscopic and white light-curves; ‘white’ refers to the parameter being free in the integrated white light-curve fit, and then fixed in the spectroscopic light-curve fit; ‘fixed’ denotes parameters that are fixed in all cases. For Gaussian priors, we list the mean and standard deviation, N(μ, σ2). For uniform priors, we list the upper and lower boundaries of the prior space, U(a, b). Gaussian-prior parameters in the astrophysical model are taken from the values of Mancini et al. (2018).
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