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Table 2
Analysis of the dispersion of the BIS and FWHM.
| Star |  |
 |
 |
 |
|---|---|---|---|---|
| [%] | [%] | |||
| HD 27969 | 1.34 ± 0.21 | 8.1 | 1.50 ± 0.24 | 22 |
| HD 80869 | 0.88 ± 0.15 | 8.3 | 1.69 ± 0.35 | 39 |
| HD 95544 | 1.11 ± 0.18 | 5.2 | 1.29 ± 0.21 | 15 |
| HD 109286 | 1.31 ± 0.16 | 6.5 | 2.13 ± 0.26 | 26 |
| HD 115954 | 1.38 ± 0.16 | 10.4 | 1.32 ± 0.15 | 25 |
| HD 211403 | 1.90 ± 0.21 | 30 | 1.26 ± 0.14 | 49 |
Notes. ⟨ σX ⟩ indicates the average error bar on the individual measurements of X. 
is the maximum fraction of the observed rv amplitude that X can have without producing a
ratio larger than one at 3 sigma; see Sect. 4.8.1 for more details on the interpretation.
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