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Table A.4
Expected maximum semi-amplitudes of the rotation induced RV signals for the stars for which a direct determination of the period was possible but the signal did not show up in the RV time series.
| Star |  |
Expected semi amp. |
|---|---|---|
| (m s−1) | ||
| GJ 4057 | −5.03 ± 0.04 | 2.7 ± 0.6 |
| GJ 548A | −4.78 ± 0.03 | 3.7 ± 0.8 |
| GJ 3997 | −4.78 ± 0.03 | 2.3 ± 0.5 |
| GJ 184 | −5.09 ± 0.04 | 2.4 ± 0.5 |
| GJ 694.2 | −4.46 ± 0.04 | 5.8 ± 1.3 |
| GJ 685 | −4.79 ± 0.04 | 3.7 ± 0.8 |
| GJ 720A | −5.03 ± 0.04 | 2.7 ± 0.6 |
| GJ 412A | −5.51 ± 0.04 | 1.4 ± 0.3 |
| GJ 15A | −5.27 ± 0.04 | 1.9 ± 0.4 |
| GJ 119 A | −4.97 ± 0.04 | 2.9 ± 0.6 |
| GJ 156.1A | −5.04 ± 0.04 | 2.6 ± 0.6 |
| GJ 9440 | −5.25 ± 0.04 | 2.0 ± 0.4 |
| GJ 521 A | −5.36 ± 0.05 | 1.7 ± 0.4 |
| NLTT 21156 | −4.58 ± 0.08 | 4.9 ± 1.1 |
| GJ 1030 | −4.84 ± 0.06 | 3.4 ± 0.8 |
| GJ 552 | −5.07 ± 0.04 | 2.5 ± 0.6 |
| GJ 476 | −5.21 ± 0.05 | 2.1 ± 0.5 |
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