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Table 6.
Expected maximum flux change from co-rotating starspots ΔFDR compared to the amplitude of the rotational modulation observed around the transit Aphot in SAP or PDC light curves.
| Planet | Transit | Data | Aphot/10−5 | ΔFDR/10−5 |
|---|---|---|---|---|
| HD189733 b | 2161 | SAP | 1454 | 16 ± 9 |
| HD189733 b | 2165 | SAP | 1454 | 34 ± 18 |
| HD189733 b | 2167 | SAP | 1454 | 64 ± 20 |
| HD189733 b | 2168 | SAP | 1260 | 113 ± 18 |
| HD189733 b | 2170 | SAP | 882 | 33 ± 11 |
| HD189733 b | 2317 | SAP | 954 | 26 ± 11 |
| HD189733 b | 2323 | SAP | 956 | 212 ± 14 |
| HD189733 b | 2326 | SAP | 832 | 28 ± 24 |
| Kepler-411 c | 117 | SAP | 1288 | 149 ± 64 |
| Kepler-411 c | 121 | SAP | 175 | 27 ± 17 |
| TOI-1268 b | 3 | SAP | 1663 | 1432 ± 370 |
| TOI-3884 b | −16 | PDC | 1468 | 4047 ± 2263 |
| TOI-3884 b | −15 | PDC | 1189 | 1984 ± 1078 |
| TOI-3884 b | 1 | PDC | 1103 | 2782 ± 1262 |
| WASP-107 b | 4 | PDC | 555 | 122 ± 21 |
| WASP-107 b | 6 | PDC | 793 | 79 ± 15 |
| WASP-107 b | 11 | PDC | 408 | 127 ± 68 |
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