Table 3.
Parameters derived by fitting the light curve with PHOEBE.
| Solution | R2 | ΣR | T2/T1 | i | e | ω |
|---|---|---|---|---|---|---|
| Nr. | (R⊙) | (R⊙) | (deg) | (deg) | ||
| 1 | 3.00 | 8.18 | 0.973 | 86.74 | 0.2854 | 18.60 |
| 2 | 3.36 | 8.40 | 1.025 | 86.52 | 0.2904 | 21.58 |
| 3 | 3.84 | 8.51 | 1.036 | 86.39 | 0.2883 | 20.43 |
| 4 | 4.27 | 8.54 | 1.043 | 86.37 | 0.2887 | 20.68 |
| 5 | 4.50 | 8.53 | 1.042 | 86.39 | 0.2886 | 20.24 |
| ⟨⟩ | 8.36 | 1.008 | 86.56 | 0.2871 | 19.64 | |
| ± | 0.18 | 0.035 | 0.18 | 0.0017 | 1.04 | |
| ⟨2+3⟩ | 8.46 | 1.030 | 86.46 | 0.2894 | 21.01 | |
Notes. The secondary radius, R2, is a free parameter. The other parameters are derived by fitting the light curve. ΣR is the sum of the two radii, R1 + R2, T2/T1 the ratio of the brightness temperatures in the TESS passband, i the inclination, e the eccentricity, and ω the longitude of periastron. The row marked with ⟨⟩ is the mean of the extremes, and the uncertainty covers the range of values. ⟨2+3⟩ denotes the mean of solutions 2 and 3.
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