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Table A.2

Spectral type, effective temperature, and rotation period of the investigated stars.

KIC Spectral type Teff [K] σTeff [K] Reference Prot [d] σProt [d] Reference Notes

3632418 F6IV 6148 111 (1) 12.591 0.036 (5) Planet host (8)
3656476 G5IV 5586 108 (1) 31.67 3.53 (6) High proper motion (9)
4914923 G1.5V 5808 92 (1) 20.49 2.82 (6)
5184732 G4V 5669 97 (1) 19.79 2.43 (6)
6106415 G0 6055 70 (2), (3)
6116048 F9IV-V 5991 124 (1) 17.26 1.96 (6)
6603624 G8IV-V 5471 128 (1)
6933899 G0.5IV 5837 97 (1)
7680114 G0V 5799 91 (1) 26.31 1.86 (6)
7976303 F8V 6119 106 (1)
8006161 G8V 5258 97 (1) 29.79 3.09 (6) High proper motion (9)
8228742 F9IV-V 6061 108 (1) 20.23 2.16 (6)
8379927 F9IV-V 5998 108 (1) 17.259 0.026 (7) Spectroscopic binary (10)
8760414 G0IV 5850 166 (1) High proper motion (11)
9025370 F8 5659 73 (2), (4)
9955598 K0V 5264 95 (1) 34.20 5.64 (6) Planet host (12)
10018963 F6IV 6145 112 (1)
10516096 F9IV-V 5928 95 (1)
10644253 G0V 5910 93 (1) 10.91 0.87 (6)
10963065 F8V 6097 130 (1) 12.444 0.172 (5) Planet host (12)
11244118 G5IV 5605 104 (1) 23.17 3.89 (6)
11295426 5796 78 (4) Planet host (13)
12009504 F9IV-V 6099 125 (1) 9.426 0.327 (7)
12258514 G0.5IV 5952 95 (1) 15.00 1.84 (6)

Notes.

(*)

If one reference is given, it applies to the spectral type and Teff. If two references are given, the first one applies to the spectral type and the second to Teff.

Reference. (1) Molenda-Żakowicz et al. (2013); (2) SIMBAD1 entry without reference; (3) Bruntt et al. (2012); (4) Pinsonneault et al. (2012); (5) McQuillan et al. (2013); (6) García et al. (2014a); (7) McQuillan et al. (2014); (8) Howell et al. (2012); (9) van Leeuwen (2007); (10) Griffin (2007); (11) Lépine & Shara (2005); (12) Marcy et al. (2014); (13) Gilliland et al. (2013).

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