Table 3.
Orbital parameters derived by the EMCEE code vs. the results from the literature.
| P | γ | K | ω | e | a | i | M2, min | Reference |
|---|---|---|---|---|---|---|---|---|
| (d) | (km s−1) | (km s−1) | (°) | (R⊙) | (°) | (M⊙) | ||
| 0.5699079 ± 0.0000068 | 8.47 ± 0.34 | 104.29 ± 0.47 | – | – | – | – | 0.37 ± 0.02 | [1] |
| 0.569899 ± 0.000001 | 7.3 ± 0.2 | 104.5 ± 0.3 | – | – | 3.1 ± 0.4 | 40 ± 6 | 0.45 | [2] |
| – | – | – | – | – | 2.53 ± 0.01 | 89.4 ± 0.6 | 0.33 | [3] |
 |
 |
 |
 |
 |
– | – | 0.36 | This work |
Notes. The parameters P, γ, K, ω, e, a, and i denote the orbital period, system velocity, the semi-amplitude for the primary star, the angle of the pericenter, the orbital eccentricity, the orbital semi-major axis, and the orbital inclination of the binary system, respectively.
References. (1) Moran et al. (1999); (2) Geier et al. (2008); (3) Schaffenroth et al. (2023).
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