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Table 3.

Same as Table 2, but for the 19 low-fsv stars in our sample.

KIC Ωrotcrit (%) Strategy Aunres/res (ppm)
003240411 67 ± 5 3 ∼500/570
003756031 / 3 ∼130/690
004939281 (*) 78 ± 17 3 ∼350/1850
006462033 85 ± 6 2 ∼60/600
007630417 66 ± 16 2 ∼160/540
008057661 59 ± 16 3 ∼50/310
008087269 / 3 ∼175/1150
008255796 3 ± 5 3 ∼280/970
008381949 76 ± 6 3 ∼135/650
008459899 8 ± 4 2 ∼145/640
009715425 (*) 83 ± 9 1 ∼2400/4700
009964614 / 2 ∼130/520
010285114 (*) / 3 ∼380/730
010536147 67 ± 8 3 ∼145/2075
011152422 (*) / 3 ∼135/540
011360704 (*) 96 ± 4 3 ∼1225/2075
011454304 / 3 ∼350/535
011971405 (*) 72 ± 8 2 ∼950/3500
012258330 73 ± 9 5 ∼155/500

Average 57 N.A. 441/1218
 – Outb. (a) 90 N.A. 907/2232
 – H.m.d. (b) 44 N.A. 186/750

Notes. The rotation rates, highest-fsv strategies, symbolic largest-amplitude ratios, and average weighted rotation rates are determined in a similar way as was done for Table 2. A suspected binary star (Lehmann et al. 2011) has its KIC identifier marked in bold. (*)Outbursting star.

(a)

Average sample properties for the outbursting stars.

(b)

Average sample properties for the high-mode-density stars.

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