Table 4
Median and 1-σ errors of the posterior PDFs deduced for the jump parameters from the individual analysis of the eclipse light curves.
| Epoch | Filter | dFocc | b | dF | W | T0 | O–C | |
| [%] | [%] | [h] | [BJDTDB-2 450 000] | [min] | ||||
|
|
||||||||
| 11 | I + z |
|
|
|
|
−0.09 ± 0.69 | ||
| 13.5 | NB2090 |
|
||||||
| 22 | I + z |
|
|
|
5546.76490 ± 0.00020 | 0.16 ± 0.29 | ||
| 27 | I + z |
|
2.721 ± 0.077 | 1.250 ± 0.018 |
|
0.15 ± 0.20 | ||
| 38 | I + z |
|
|
|
5559.78038 ± 0.00021 | −0.07 ± 0.30 | ||
| 38 | Gunn-r′ |
|
|
|
5559.78092 ± 0.00016 | 0.71 ± 0.22 | ||
| 40.5 | z ′ |
|
||||||
| 43 | I + z |
|
2.60 ± 0.17 |
|
5563.84773 ± 0.00023 | −0.12 ± 0.33 | ||
| 49 | I + z |
|
|
|
|
−0.54 ± 0.26 | ||
| 51.5 | NB1190 |
|
||||||
| 59 | I + z |
|
|
1.219 ± 0.029 | 5576.86380 ± 0.00015 | 0.51 ± 0.22 | ||
| 65 | I + z |
|
|
1.212 ± 0.014 |
|
−0.28 ± 0.19 | ||
| 70 | I + z |
|
|
|
|
0.59 ± 0.56 | ||
| 76 | Gunn-r′ |
|
|
|
|
0.05 ± 0.25 | ||
| 87 | Gunn-r′ |
|
|
|
5599.64042 ± 0.00017 | −0.57 ± 0.25 | ||
| 97 | I + z |
|
|
|
|
−0.63 ± 0.22 | ||
| 124 | I + z |
|
|
1.213 ± 0.014 |
|
0.79 ± 0.20 | ||
| 126.5 | z ′ |
|
||||||
| 140 | I + z |
|
|
1.223 ± 0.018 |
|
−0.86 ± 0.25 | ||
| 141 | I + z |
|
|
1.240 ± 0.020 |
|
0.18 ± 0.27 | ||
| 148.5 | z ′ |
|
||||||
| 152 | I + z |
|
2.82 ± 0.11 |
|
|
−1.48 ± 0.33 | ||
| 154.5 | z ′ |
|
||||||
| 168 | I + z |
|
2.42 ± 0.12 |
|
|
−0.36 ± 0.32 | ||
| 173 | I + z |
|
|
|
5669.59946 ± 0.00025 | −0.58 ± 0.36 | ||
| 189 | I + z |
|
|
|
|
0.61 ± 0.30 | ||
| 200 | I + z |
|
|
|
|
0.05 ± 0.19 | ||
| 202.5 | z ′ |
|
||||||
| 211 | I + z |
|
|
|
|
0.47 ± 0.22 | ||
| 243 | I + z |
|
|
|
|
1.57 ± 0.81 | ||
Notes. For each light curve, this table shows the epoch based on the transit ephemeris presented in H11, the filter, and the derived values for the occultation depth, impact parameter, transit depth, transit duration, and transit time of minimum light. The last column shows for the transits the difference (and its error) between the measured timing and the one deduced from the best-fitting transit ephemeris computed by linear regression, T(N) = 2 455 528.868289(0.000072) + N × 0.81347728(0.00000060) BJDTDB.
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