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Table 3.

Results of the KR of the RV residuals of the keplerian model that does not include the linear correlation between the RV and the stellar chromospheric index for our stars.

Star name Indicator Nc σ [m s−1] σKR res [m s−1] ht [d] hx v F α
HD 23596 BIS 25 3.384 1.636 85.161 1.655e-03 8.879 6.289 0.001154
HD 23596 ΔV 25 3.384 1.606 85.161 1.931e-03 10.182 5.176 0.003308
HD 23596 Vasy(mod) 25 3.384 1.556 85.161 2.459e-03 11.679 4.303 0.008842
HD 23596 FWHM 25 3.384 1.665 85.161 1.815e-03 8.284 6.748 0.000786
HD 89307 BIS 19 3.765 1.446 84.339 1.777e-03 8.642 7.064 0.003759
HD 89307 Vasy(mod) 19 3.765 1.187 84.339 1.815e-03 8.046 12.582 0.000316
HD 106252 BIS 43 2.365 1.269 79.651 8.857e-04 19.965 2.871 0.009616
HD 188015 21 4.409 1.724 110.264 1.295e-02 9.138 7.392 0.001748
HD 188015 FWHM 21 4.409 1.902 110.264 3.183e-03 8.384 6.868 0.002084
HD 190228 Vasy(mod) 43 2.619 1.435 41.111 8.937e-04 17.415 3.486 0.002610
XO2S BIS 42 3.538 1.537 72.829 3.774e-03 19.499 4.969 0.000292

Notes. Only the cases with significant correlations, that is α < 0.01, are listed (see the text).

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