Table 3
Parameters of the best fit with a binary model including a spotted secondary and consistent with ABLDR2.
| LC option | f1 | f2 | i (°) | Spot | χ2 | |||
|---|---|---|---|---|---|---|---|---|
| long. (°) | radius (°) | dim | ||||||
| I | 0.646 | 0.980 | 28.4 | 95.6 | 7.6 | 0.65 | 28.3 | |
| II | 0.464 | 0.980 | 27.0 | 212.9 | 22.9 | 1.12 | 27.9 | |
| III | 0.646 | 0.980 | 29.2 | 203.4 | 51.9 | 1.03 | 1.6 | |
Notes. The corresponding fits are illustrated in Fig. 11. For comparison, the 
values for the full parameter space that we explored are 28.1, 27.1, and 1.5 for lightcurve options I, II, and III, respectively. Spot longitudes of 90° and 270° correspond to the trailing and leading side of the secondary star, respectively.
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