Table 2
Input system parameters of HAT-P-32 b used for the secondary eclipse model.
| Parameter | Value |
|---|---|
| i (°) | 88.90 |
| a∕R⋆ | 6.05 |
| Rp∕R⋆ | 0.1508 |
| e | 0.0 |
| ω (°) | 0.0 |
| T0 (BJDTDB) | 2 454 420.447187 |
| P (days) | 2.1500080 |
Notes. From first to last row, it lists the orbital inclination i, orbital semimajor axis a∕R⋆, planet-star radius ratio Rp∕R⋆, eccentricity of the orbit e, argument of periastron ω, zero point of the transit ephemeris T0, and orbital period P. The parameters were adopted from Nikolov et al. (2018) and Tregloan-Reed et al. (2018) and were kept fixed in the analysis.
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