Table 3
Orbital parameters for systems for which the periastron has been monitored with the Hermes spectrograph.
| Star | n RV | P orbit | e | Ω | K | γ | T 0 | Eclipse |
| KIC | [d] | [rad] | [km s-1] | [km s-1] | [HJD] | duration | ||
|
|
||||||||
| 9151763 | 24 | 437.51 ± 0.03 | 0.73 ± 0.01 | 3.03 ± 0.01 | 16.20 ± 0.04 | –92.89 ± 0.03 | 2 455 949.64 ± 0.06 | |
| 5039392 | 13 | 236.70 ± 0.02 | 0.44 ± 0.01 | 4.96 ± 0.01 | 22.6 ± 0.2 | –14.96 ± 0.05 | 2 454 874.2 ± 0.27 | |
| 9540226⋆ | 31 | 175.43 ± 0.01 | 0.39 ± 0.01 | 0.07 ± 0.01 | 23.32 ± 0.04 | –12.37 ± 0.02 | 2 456 425.89 ± 0.09 | P: 4 d; S: 3 d |
| 8210370 | 16 | 153.50 ± 0.01 | 0.70 ± 0.01 | 1.17 ± 0.01 | 12.96 ± 0.36 | –0.76 ± 0.08 | 2 454 937.35 ± 0.01 | |
| 10614012⋆ | 22 | 132.13 ± 0.01 | 0.71 ± 0.01 | 1.23 ± 0.01 | 24.68 ± 0.03 | –0.92 ± 0.02 | 2 454 990.48 ± 0.01 | 1 d |
| 9163796 | 17 | 121.30 ± 0.01 | 0.69 ± 0.01 | 0.00 ± 0.01 | 35.64 ± 0.01 | –11.05 ± 0.01 | 2 456 409.60 ± 0.01 | |
| 2444348 | 17 | 103.50 ± 0.01 | 0.48 ± 0.01 | 4.30 ± 0.01 | 4.76 ± 0.02 | 14.47 ± 0.01 | 2 454 947.74 ± 0.09 | |
| 5006817 | 70 | 94.812 ± 0.002 | 0.7069 ± 0.0002 | 4.0220 ± 0.0005 | 11.709 ± 0.005 | –14.021 ± 0.002 | 2 456 155.924 ± 0.002 | |
| 8144355 | 19 | 80.55 ± 0.01 | 0.76 ± 0.01 | 2.79 ± 0.01 | 9.44 ± 0.04 | 0.02 ± 0.03 | 2 455 914.43 ± 0.02 | |
| 9408183 | 7 | 49.70 ± 0.01 | 0.42 ± 0.01 | 0.17 ± 0.01 | 37.17 ± 0.04 | –14.37 ± 0.01 | 2 454 989.80 ± 0.01 | |
| 2720096 | 13 | 26.70 ± 0.01 | 0.49 ± 0.01 | 6.11 ± 0.01 | 2.28 ± 0.03 | 9.92 ± 0.01 | 2 454 990.67 ± 0.05 | |
| 8095275 | 25 | 23.00 ± 0.01 | 0.32 ± 0.01 | 2.19 ± 0.01 | 10.50 ± 0.06 | –8.58 ± 0.03 | 2 454 971.02 ± 0.03 | |
| 2697935⋆ | 27 | 21.50 ± 0.01 | 0.41 ± 0.02 | 2.33 ± 0.06 | 26.5 ± 0.6 | –74.4 ± 0.4 | 2 454 990.9 ± 0.1 | 0.1 d |
| 8912308 | 28 | 20.17 ± 0.01 | 0.23 ± 0.01 | 3.34 ± 0.01 | 30.78 ± 0.02 | –52.69 ± 0.01 | 2 454 994.06 ± 0.01 | |
Notes. Number of radial velocity measurements, nRV; orbital period Porbit; eccentricity e; argument of periastron Ω; radial velocity amplitude K; velocity of the system γ; and zero point T0. The duration of the eclipse is given. P and S indicate the primary and secondary eclipses, respectively.
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