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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 |
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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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