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Table 2.

Rotation rates (Ωrotcrit, Pedersen et al. 2021), highest-fsv pre-whitening strategies, and symbolic largest-amplitude ratio (Aunres/res) for the 19 high-fsv stars, if applicable.

KIC Ωrotcrit (%) Strategy Aunres/res (ppm)
003459297 55 ± 6 2 ∼135/4600
003839930 / 2 ∼330/10 000
003865742 88 ± 10 2 ∼160/8750
004930889 60 ± 12 3 ∼310/8000
004936089 16 ± 7 3 ∼80/5700
005084439 / 2 ∼175/3650
005309849 46 ± 14 3 ∼65/3400
005941844 39 ± 4 3 ∼300/14 000
006352430 50 ± 11 2 ∼350/7400
006780397 70 ± 24 3 ∼26/440
007760680 25 ± 5 5 ∼390/9800
008324482 / 2 ∼175/2000
008714886 60 ± 18 2 ∼155/2150
008766405 77 ± 10 3 ∼110/1750
009020774 51 ± 10 2 ∼75/7700
009227988 / 3 ∼170/2200
010220209 / 2 ∼44/1300
010526294 4 ± 3 3 ∼2000/14 500
010658302 / 3 ∼620/3000

Average 29 (a) N.A. 300/5807

Notes. Rotation rates are obtained from averaging over eight theories of core-boundary and envelope mixing by Pedersen et al. (2021). The highest-fsv pre-whitening strategy noted in the ‘Strategy’ column is that strategy which delivers the highest-fsv light curve regression model among the models generated by all five strategies. The symbolic largest-amplitude ratio Aunres/res consists of the (approximate) amplitude of the largest-amplitude unresolved signal in the LS periodogram of the light curve subtracted by the highest-fsv regression model, symbolically divided by the amplitude of the largest-amplitude resolved signal in the LS periodogram of the original light curve. Known binary stars (Pápics et al. 2013, 2017) have their KIC identifiers marked in boldface.

(a)

Average weighted rotation rate, where the inverse variances () are used as weights.

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