Table 6
Comparison of periods returned by our method with spot periods from previously studied Kepler stars.
| KIC | 8 429 280 | 7 985 370 | 7 765 135 | 5 110 407 |
|
|
||||
| P1out | 1.16194 | 2.84359 | 2.55393 | 3.61073 |
| P2out | 1.21012 | 3.09043 | 2.39581 | 3.42325 |
| α out | 0.040 | 0.080 | 0.062 | 0.052 |
|
|
||||
| P1closest | 1.16298a | 2.8428b | 2.5645c | − |
| P2closest | 1.20430a | 3.0898b | 2.4018c | 3.4693d |
| α closest | 0.034 | 0.080 | 0.063 | − |
|
|
||||
| dΩ / Ωeq | 0.049 | 0.080 | 0.067 | 0.053d |
Notes.The periods closest to P1out (P2out) are called P1closest (P2closest).
Periods from a seven-spots fit (Frasca et al. 2011).
Periods from seven-spots fit (Fröhlich et al. 2012).
Periods from nine-spots fit (Fröhlich et al. 2012).
Period and DR coefficient from Roettenbacher et al. (2013).
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