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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