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Table 2.

Results of the KR of the RV residuals of the keplerian model including a 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 2.642 1.445 85.161 1.655e-03 8.879 4.500 0.005952
HD 23596 ΔV 25 2.642 1.347 85.161 1.931e-03 10.182 4.269 0.007890
HD 23596 FWHM 25 2.642 1.411 85.161 1.815e-03 8.284 5.401 0.002504
HD 89307 BIS 19 3.775 1.467 84.339 1.777e-03 8.642 6.862 0.004178
HD 89307 Vasy(mod) 19 3.775 1.187 84.339 1.815e-03 8.046 12.648 0.000309
HD 106252 BIS 43 2.350 1.259 79.651 8.857e-04 19.965 2.884 0.009355
HD 155358 43 1.947 1.089 67.353 2.200e-03 17.987 3.095 0.005702
HD 188015 FWHM 21 3.945 1.885 110.264 3.183e-03 8.384 5.300 0.006108
HD 190228 Vasy(mod) 43 2.621 1.437 41.111 8.937e-04 17.415 3.482 0.002628
XO2S BIS 42 3.534 1.513 70.129 3.774e-03 19.207 5.312 0.000171

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

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