Table B.3
Measured υsini⋆ based on the SOPHIE CCFs.
KIC | KOI | υsini⋆ | σ υsini⋆ | Method |
[km s-1] | [km s-1] | |||
|
||||
11974540 | 129 | 18.98 | 0.03 | RotPro |
8506766 | 138 | 22.1 | 0.1 | RotPro |
10666242 | 198 | 4.1 | 1.2 | Bo10 |
3937519 | 221 | 4.4 | 1.2 | Bo10 |
11442793 | 351 | 4.1 | 1.2 | Bo10 |
6603043 | 368 | 86.5 | 0.6 | RotPro |
6471021 | 372 | 4.1 | 1.2 | Bo10 |
5779852 | 449 | 7.4 | 1.2 | Bo10 |
8890783 | 464 | 4.8 | 1.2 | Bo10 |
10395543 | 531 | 6.2 | 1.2 | Bo10 |
11773022 | 620 | 5.7 | 1.2 | Bo10 |
3247268 | 1089 | 3.5 | 1.2 | Bo10 |
6470149 | 1230 | 4.7 | 1.2 | Bo10 |
6665223 | 1232 | 4.1 | 1.2 | Bo10 |
8631160 | 1271 | 4.6 | 1.2 | Bo10 |
7303287 | 1353 | 5.3 | 1.2 | Bo10 |
8958035 | 1391 | 5.1 | 1.2 | Bo10 |
9425139 | 1411 | 4.6 | 1.2 | Bo10 |
11122894 | 1426 | 2.8 | 1.2 | Bo10 |
11075279 | 1431 | 4.6 | 1.2 | Bo10 |
7449844 | 1452 | 36.2 | 0.2 | RotPro |
11702948 | 1465 | 5.4 | 1.2 | Bo10 |
11909686 | 1483 | 3.6 | 1.2 | Bo10 |
5475431 | 1546 | 5.9 | 1.2 | Bo10 |
10028792 | 1574 | 3.3 | 1.2 | Bo10 |
10005758 | 1783 | 3.0 | 1.2 | Bo10 |
2975770 | 1788 | 6.2 | 1.2 | Bo10 |
6716021 | 2679 | 29.8 | 0.2 | RotPro |
12735740 | 3663 | 3.4 | 1.2 | Bo10 |
4150804 | 3678 | 4.5 | 1.2 | Bo10 |
9025971 | 3680 | 3.9 | 1.2 | Bo10 |
2581316 | 3681 | 5.9 | 1.2 | Bo10 |
10795103 | 3683 | 8.9 | 1.2 | Bo10 |
7017372 | 3689 | 2.4 | 1.2 | Bo10 |
10735331 | 3720 | 24.7 | 0.1 | RotPro |
6775985 | 3780 | 5.5 | 1.2 | Bo10 |
9533489 | 3783 | 71.7 | 0.1 | RotPro |
7813039 | 3787 | 3.7 | 1.2 | Bo10 |
4769799 | 5086 | 4.6 | 1.2 | Bo10 |
5179609 | 5132 | 4.9 | 1.2 | Bo10 |
7377343 | 5384 | 43.6 | 0.3 | RotPro |
9724993 | 5708 | 7.3 | 1.2 | Bo10 |
12645761 | 5976 | 4.8 | 1.2 | Bo10 |
9221398 | 6066 | 3.9 | 1.2 | Bo10 |
5034333 | 6124 | 51.3 | 0.8 | RotPro |
5629353 | 6132 | 9.3 | 1.2 | Bo10 |
8197761 | 6175 | 4.8 | 1.2 | Bo10 |
1147460 | 6235 | 5.1 | 1.2 | Bo10 |
12470041 | 6251 | 19.1 | 0.3 | RotPro |
Notes. The instrumental resolution of SOPHIE corresponds to a υsini⋆ of ~4 km s-1 for a solar-like star. Therefore, υsini⋆ vales lower than 4 km s-1 should be considered as upper limits.
Notes.Bo10 refers to the method described in Boisse et al. (2010) to measure the υsini⋆ from the Gaussian width of the SOPHIE CCF. RotPro means that the υsini⋆ was measured on the CCF using a rotation profile, as described in Santerne et al. (2012a).
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