Eclipsing binaries and fast rotators in the Kepler sample - Characterization via radial velocity analysis from Calar Alto

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Table 4

Upper limits for the mass of the transiting companion to KOIs with large vsini values (fast rotators, Group B).

Group B − Fast rotators

KOI	vsini	K	V_sys	σ_K
		(km s^-1)	(km s^-1)	(km s^-1)	(M_Jup)

12.01	70 ± 5 ^a	0.140 ± 1.425	−18.6 ± 1.1	1.565	25.2 ± 3.7
131.01	26^†^b	1.400 ± 1.995	−9.0 ± 1.8	3.395	35.8 ± 5.0
366.01	35 ± 2 ^c	0.027 ± 0.255	8.5 ± 0.2	0.282	8.70 ± 0.59
625.01	25 ± 2 ^c	0.120 ± 0.510	−25.87 ± 0.42	0.630	14.1 ± 1.6
972.01	120 ± 5 ^c	2.200 ± 3.300	−14.1 ± 2.4	5.500	106.8 ± 2.6
3728.01	55^†^a	4.810 ± 2.775	−52.6 ± 2.4	7.585	111.6 ± 6.3

Notes.

^(†)

No uncertainties provided.

^(a)

Values obtained from the analysis of TrES spectra by Byerla.

^(b)

Values obtained from the analysis of Lick spectra by Isaacson.

^(c)

Values obtained from the analysis of McDonald or TrES spectra by Quinn.

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