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Table 4

Table of the multiple stars in our sample.

KID Prot [days] error Prot [days] Sph,k = 5 error Sph,k = 5 Type Reference

2010607 17.60 3.89 264.73 5.06 EB Kirk et al., in prep.
3427720 13.94 2.15 106.72 2.27 Mult. SIMBAD
4586099 10.76 1.94 137.62 3.25 Mult. SIMBAD
5021689 –1.00 0.00 –1.00 0.00 Mult. SIMBAD
7510397 –1.00 0.00 –1.00 0.00 Mult. SIMBAD
7938112 0.84 0.07 214.08 19.03 Seis/Pol This study
8360349 –1.00 0.00 –1.00 0.00 Mult. SIMBAD
8379927 16.99 1.35 1340.50 23.44 SB2 Griffin 2007
9025370 13.31 1.30 171.69 3.63 SB2 Thygesen et al. (2014)
9139151 10.96 2.22 187.29 4.22 Mult. SIMBAD
9139163 6.10 0.47 71.23 2.32 Mult. SIMBAD
9693187 –1.00 0.00 –1.00 0.00 SB2 Thygesen et al. (2014)
9908400 17.12 1.26 530.12 10.29 Mult. SIMBAD
10124866 17.59 2.27 248.23 4.38 Mult. SIMBAD
11453915 23.85 1.55 75.45 1.38 EB Kirk et al., in prep.

Notes. Columns are the same as in Table 3, except for the column “Type” in which the type of multiple star is given (EB: eclipsing binary, SB2: double-lined spectroscopic binary, Mult: multiple in SIMBAD database, Seis/Pol: seismic binary or pollution by a nearby red giant) and the column “Reference”, which explains from which paper or website this classification comes from. Stars for which no rotation period was derived have Prot = ⟨ Sph,k = 5 ⟩ = −1. The star for which KID shows a

(†)

is a KOI.

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