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Table 1
Best-fitting parameters of the Keplerian solution fitted to the RV measurements of EX Lup (with RVlin, using the combined FEROS and HARPS dataset).
| Parameter | Unit | Value |
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|
||
| Period | day | 7.417 ± 0.001 |
| RV semi-amplitude | km s-1 | 2.18 ± 0.10 |
| Eccentricity | ... | 0.23 ± 0.05 |
| Longitude of periastron | ° | 96.8 ± 11.4 |
| Epoch of periastron passage | JD | 2 455 405.112 ± 0.224 |
| RV offset | km s-1 | –0.52 ± 0.07 |
| FAPa | ... | 6.7×10-27 |
|
|
||
| msinib | M Jupiter | 14.7 ± 0.7 |
| semi-major axisb | au | 0.063 ± 0.005 |
Notes.
(a)
False alarm probability of the Keplerian fit as defined by Cumming (2004).
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