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Table 1
Orbital (P, K, e, ω, λ0) and physical (a, m sin i) parameters obtained from the MCMC performed on the different RV time series of HD 192310 for a 2-Keplerian fit model.
DRS | YV1 | YV2 | ||||
---|---|---|---|---|---|---|
Parameter (unit) | planet b | planet c | planet b | planet c | planet b | planet c |
P (days) | ||||||
K (m s−1) | ||||||
e() | ||||||
ω (º) | ||||||
λ0 (º) | ||||||
a (AU) | ||||||
m sin i (M⊕) |
Notes. The reference date is BJD = 2 455 500 and the stellar mass is taken as M* = 0.82 M⊙ (Ramírez et al. 2013).
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