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Table 1
The candidate sample that survives the impact parameter cut.
| WinID+CoRoTID | P |
|
b |
|
|
2σ | |
|
|
|||||||
| 1126 0102890318 | 1.51 | 0.14 | 0.43 | –0.16 | 4.93 | 14% | |
| 0330 0102912369 | 9.20 | 0.10 | 0.18 | –0.13 | 16.96 | 31% | |
| 0203 0102825481 | 5.17 | 0.18 | 0.62 | 0.04 | 13.09 | 30% | |
| 1712 0102826302 | 2.77 | 0.05 | 0.60 | –0.88 | 4.27 | 93% | |
| 4108 0102779966 | 7.37 | 0.07 | 0.80 | –0.06 | 15.41 | 95% | |
|
|
|||||||
| (R2/R1) versus ρ ∗ | |||||||
| 4617 0102753331 | 19.76 | 0.19 | 0.10 | –1.42 | 10.47 | 20% | |
| 2430 0102815260 | 3.59 | 0.10 | 0.24 | –0.81 | 5.36 | 44% | |
| 4073 0102863810 | 15.00 | 0.18 | 0.36 | –0.08 | 24.40 | 67% | |
| 1736 0102855534 | 21.72 | 0.11 | 0.43 | –1.24 | 12.77 | 62% | |
| 3724 0102759638 | 12.33 | 0.10 | 0.50 | –1.33 | 8.17 | 78% | |
Notes. The last six sources are excluded using a second cut because the fitted host star density indicates a secondary radius R2 > 2 RJup. The last column indicates the 2σ upper limit to the blended light fraction k.
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