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Table 3
Stars with the largest RV variability, which are candidates to host substellar companions.
| Object | V | B − V | RV (km s-1) | σRV (km s-1) |
|
|
||||
| Y401 | 13.7 | 0.566 | 33.203 | 0.058 |
| Y673 | 14.4 | 0.665 | 33.766 | 0.099 |
| Y1051 | 14.1 | 0.595 | 33.290 | 0.130 |
| Y1587 | 14.2 | 0.600 | 33.434 | 0.063 |
| Y1722 | 14.2 | 0.560 | 34.460 | 0.098 |
| Y1788 | 14.4 | 0.622 | 34.150 | 0.048 |
| Y1955 | 14.2 | 0.589 | 33.192 | 0.050 |
| Y2018 | 14.6 | 0.631 | 31.953 | 0.086 |
| S488 | 8.9 | 1.550 | 32.910 | 0.089 |
| S815 | 12.9 | 0.497 | 33.326 | 0.378 |
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