Table 2
Summary of the seismic solar analogue observations.
| KIC | V | N | ToT | ΔT |
|
ΔRV | Comment | ||
| [mag] | [hrs] | [days] | [km s-1] | [km s-1] | |||||
|
|
|||||||||
| 3241581⋆ | 10.35±0.04 | 24 | 9.3 | 709.1 | −30.68 | 0.96 | binary | ||
| 3656476 | 9.55±0.02 | 6 | 2.5 | 351.1 | −13.23 | 0.14 | |||
| 4914923 | 9.50±0.02 | 7 | 2.1 | 297.3 | −31.16 | 2.11 | binary | ||
| 5084157 | 11.56±0.12 | 10 | 5.2 | 300.1 | −19.66 | 0.21 | |||
| 5774694 | 8.37±0.01 | 7 | 1.3 | 348.1 | −17.67 | 0.16 | |||
| 6116048 | 8.47±0.01 | 5 | 1.0 | 347.2 | −53.28 | 0.17 | |||
| 6593461 | 11.22±0.10 | 9 | 4.1 | 296.2 | −35.39 | [0.37] | large scatter | ||
| 7296438 | 10.13±0.03 | (+2) 4 | 1.5 | 350.2 | −2.08 | 16.65 | binary (KOI 364.01) | ||
| 7680114 | 10.15±0.04 | 8 | 3.4 | 351.0 | −58.96 | 0.180 | |||
| 7700968 | 10.37±0.04 | (+2) 4 | 1.4 | 299.1 | +39.47 | 27.62 | binary | ||
| 9049593 | 10.35±0.04 | 4 | 1.5 | 299.1 | −21.02 | 0.24 | |||
| 9098294 | 9.91±0.03 | 7 | 2.6 | 346.1 | −55.78 | 41.35 | binary | ||
| 10130724 | 12.03±0.19 | 7 | 2.8 | 299.1 | −54.51 | 2.12 | binary | ||
| 10215584 | 10.62±0.05 | 6 | 2.7 | 337.0 | −11.02 | 0.25 | |||
| 10644253 | 9.26±0.02 | 14 | 5.9 | 416.0 | −19.01 | 0.18 | |||
| 10971974 | 11.05±0.07 | 4 | 1.6 | 300.1 | −34.58 | 0.27 | |||
| 11127479 | 11.21±0.09 | 5 | 2.1 | 300.2 | −29.33 | 0.30 | KOI 2792.01, large scatter | ||
| 11971746 | 11.00±0.07 | 8 | 3.6 | 301.0 | −44.20 | 0.22 | |||
Notes. The star identifier in the Kepler input catalogue (KIC), apparent magnitude in Johnson V, number N of spectra (in brackets the number of additional spectra with S/N only high enough to determine the radial velocity), total accumulated time on target (ToT), the time base ΔT covered by the observations, the mean radial velocity (), and the difference between the positive and negative extrema of the measured RV values and their internal error, and a comment on the star/system. KOI stands for Kepler Objects of Interests and indicates planet host star candidates.
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