Table 1
Orbital parameters of the best-fit Keplerian model to the combined pyodine Lick and SONG RVs of the HIP 36616 system.
| Parameter | HIP 36616 Ab | HIP 36616 B |
|---|---|---|
| K (m s−1) | 131.20 ± 2.03 | 4009.29 ± 5.54 |
| P (days) | 300.01 ± 0.08 | 11256.53 ± 111.40 |
| e | 0.05 ± 0.01 | 0.72 ± 2 × 10−3 |
| ω (deg) | 119.87 ± 17.31 | 149.61 ± 0.12 |
| M0 (deg)(a) | 304.56 ± 17.37 | 255.23 ± 1.05 |
| a (au) | 1.09 | 13.23 |
| m sin i (Mjup)(b) | 6.64 | 554.94 |
| σjit(m s−1) | 17.26 | |
| rms (m s−1) | 18.05 | |
| NRV data | 191 | |
Notes. (a)The mean anomalies are calculated at the first observational epoch, t0 = 2451482.03 JD. (b)For the mass and semi-major axis calculation, a primary mass of mA = 1.9 ± 0.2 M⊙ is used (see Ortiz et al. 2016).
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