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Table 4
All models fit to the Spitzer data alone.
| Parameter | Units | Prior | Sinusoidal (ϕ = 0) | Model Name Sinusoidal (ϕ free) | Two temp. |
|---|---|---|---|---|---|
| t0 | BJDtdb-2457744.0 d | N(0.07160,0.00022) |  |
 |
 |
| Rp/R* | – | N(0.02037,0.00046) |  |
 |
 |
| a/R* | – | N(2.292,0.056) |  |
 |
 |
| cos i | – | N(0.064532,0.064) |  |
 |
 |
| A | ppm | u(0,400) |  |
 |
– |
| fp/f* | ppm | u(0,400) |  |
 |
– |
| ϕ | degrees | u(−180°, 180°) | – |  |
– |
| T* | K | N(4599,79) | – | – |  |
| Tp,n | K | u(0,4599) | – | – |  |
| Tp,d | K | u(0,4599) | – | – |  |
| ΔBIC | 0 | 8.8 | 9.6 |
Notes. The Gaussian priors on t0, Rp/R*, a/R* cos i and T* are based on the values reported in Malavolta et al. (2018). The orbital period P was fixed in these runs to P = 0.2803244 days (Malavolta et al. 2018). N and u denote a Gaussian and uniform prior, respectively.
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