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Table 1
Starspot parameters as fitted by a Gaussian model on the residual light curves of the second transit (T2/B and T2/R light curves, Fig. 3).
| T2/B | T2/R | Unit | |
|
|
|||
| δ | 4.9 ± 0.8 | 3.3 ± 0.3 | mmag |
| t0 | 8.07 ± 0.16 | 8.12 ± 0.09 | orbital phase %0 |
| 44.71 ± 0.36 | 44.83 ± 0.20 | minutes from T1 | |
| 0.848 ± 0.007 | 0.851 ± 0.004 | transit phase | |
| σ | 1.07 ± 0.19 | 1.10 ± 0.11 | orbital phase %0 |
| 2.44 ± 0.43 | 2.50 ± 0.24 | minutes | |
| FWHM | 5.7 ± 1.0 | 5.9 ± 0.6 | minutes |
Notes. The transit phase is calculated by assuming the total duration of the eclipse (T1−T4, Kipping 2010), in our case 52.4 min. The FWHM is calculated from the Gaussian σ as 
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