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Table 2

SOPHIE measurements of the planet-host star KOI-3680.

BJDUTC RV ± 1 σ Bisect.a Exp. S/Nb
−2 450 000 (km s−1) (km s−1) (km s−1) (s)
6900.5292 −44.880 0.017 −0.069 3600 16.2
6935.3558 −45.082 0.024 0.002 3600 16.3
6948.3726 −45.020 0.012 −0.044 3600 23.2
6975.3101 −44.923 0.016 −0.018 3600 20.0
6982.3470 −44.919 0.016 −0.054 3600 21.9
7107.6489 −44.878 0.026 0.002 3164 18.2
7192.5683 −44.912 0.020 0.005 3600 16.7
7211.4976 −44.922 0.034 −0.027 3600 11.9
7219.4596 −45.063 0.030 −0.088 2452 12.4
7225.4649 −45.016 0.015 −0.017 3600 19.8
7241.4781 −44.951 0.019 −0.027 3600 18.1
7246.4579 −44.948 0.022 −0.051 3600 16.1
7261.3529 −44.905 0.017 −0.047 3600 18.3
7265.4376 −44.917 0.019 0.026 3600 18.1
7276.4394 −44.913 0.014 0.024 3600 17.3
7303.3809 −44.871 0.022 0.050 3600 13.5
7334.3829 −44.929 0.025 −0.034 3443 17.4
7346.2494 −44.988 0.038 0.039 2704 10.8
7352.2475 −44.954 0.032 −0.046 3600 14.1
7359.2618 −45.063 0.015 −0.032 3600 19.1
7379.2595 −44.952 0.036 −0.002 2801 15.0
7607.4763 −44.871 0.016 −0.054 3600 15.8
7623.5069 −44.884 0.022 −0.029 3600 16.0
7628.5428 −44.951 0.020 −0.030 3600 14.4
7659.3588 −44.980 0.019 −0.085 3600 14.3

Notes. (a) Bisector spans; error bars are twice those of the RVs. (b)Signal-to-noise ratio per pixel at 550 nm.

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