Table 3.
Periods detected in the K2 light curve.
| GLS | GLSp | WWZ | |||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| N | Frequency | Period | Ident. | N | Frequency | Period | Ident. | N | Frequency | Period | Ident. |
| [d−1] | [d] | [d−1] | [d] | [d−1] | [d] | ||||||
| F1 | 0.0405 [1] | 24.7 ± 0.6 | – | F1 | 0.0402 [1] | 24.85 ± 0.61 | – | F1 | 0.0395 [1] | 25.3 ± 5.4 | – |
| F2 | 0.0608 [2] | 16.4 ± 0.2 | – | F2 | 0.0521 [3] | 19.21 ± 0.20 | – | F2 | 0.0610 [2] | 16.4 ± 1.8 | – |
| F3 | 0.1406 [3] | 7.1 ± 0.4 | – | F3 | 0.0622 [2] | 16.07 ± 0.25 | – | F3 | 0.1000 [5] | 10.0 ± 1.0 | – |
| F4 | 0.1812 [5] | 5.5 ± 0.2 | F1 + F3 | F4 | 0.1410 [4] | 7.10 ± 0.40 | – | F4 | 0.1408 [4] | 7.1 ± 0.5 | F1 + F3 |
| F5 | 0.1989 [4] | 5.0 ± 0.2 | F2 + F3 | F5 | 0.1980 [5] | 5.05 ± 0.20 | F2 + F4 | F5 | 0.1923 [3] | 5.2 ± 0.5 | F2 + F4 |
| F6 | 0.2205 [7] | 4.5 ± 0.0* | – | F6 | 0.3462 [6] | 2.90 ± 0.00 | F4 + F5 | – | – | – | – |
| F7 | 0.3459 [6] | 2.9 ± 0.0* | F3 + F4 | – | – | – | – | – | – | – | – |
Notes. Results of the analysis of three methods: GLS, GLSp, and WWZ, arranged by decreasing period in each column. The number in brackets [N] denotes the rank of the period by detected power. An asterisk (*) indicates an uncertainty of less than 0.04 days. In this and the following tables, persistent periods detected in all datasets are highlighted in bold.
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