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Table 2

Summary of RV observations.

Star HET/HRSTNG/HARPS-N
OPtotal Kosc OPHET K rBIS p No OPTNG K rBIS p No
BD+02 3497 3693 3.82 2825 72.4 7.0 -0.12 0.70 12 827 65.2 2.2 -0.47 0.05 18
BD+48 740 3492 9.37 2594 116.0 5.5 0.11 0.61 25 962 163.5 1.4 0.33 0.21 16
HD 181368 2981 1.65 2221 3908.4 6.1 -0.13 0.73 9 769 1776.4 1.6 0.16 0.53 18
HD 188214 3333 12.33 1873 24.8 5.0 -0.16 0.84 4 977 82.4 2.6 -0.15 0.62 14
HD 238914 3944 11.27 2935 121.3 5.8 -0.15 0.20 71 769 98.7 1.2 0.33 0.23 15
TYC 0684-00553-1 2340 11.54 1588 138.0 7.2 0.53 0.14 9 834 91.3 3.4 0.39 0.11 18
TYC 3105-00152-1 2868 8.77 2065 137.2 5.7 -0.12 0.70 14 827 123.2 2.3 0.21 0.36 22
TYC 3263-02180-1 3320 12.61 2408 131.7 8.9 0.15 0.67 10 977 137.8 1.6 0.47 0.04 19
TYC 3300-00133-1 3940 2.95 1742 56.1 6.2 0.06 0.96 3 592 45.1 3.3 -0.14 0.68 11
TYC 3318-01333-1 3514 3.19 2630 306.0 5.5 0.46 0.14 12 962 241.8 2.2 -0.40 0.12 16
TYC 3663-01966-1 2940 14.70 2500 91.7 7.7 -0.32 0.16 20 650 67.7 3.2 -0.25 0.43 12
TYC 3930-00681-1 3769 4.49 1068 7.2 5.5 1.00 0.00 2 496 80.0 3.1 0.34 0.30 11

Notes. OPtotal denotes the total observation period in days, OPHET, OPTNG are observing periods for the HET and TNG, respectively, Kosc is the amplitude of solar-like oscillations (Kjeldsen & Bedding 1995) in m s−1, K denotes the amplitude of the observed radial velocities defined as RVmaxRVmin, in m s −1, is the average RV uncertainty in m s−1, and rBIS is the linear correlation coefficient between the RV and BIS.

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