Table 7
Best-fitted solution for the planetary system orbiting HD 21693.
Param. | Units | HD21693b | HD21693c |
---|---|---|---|
P | (d) | 22.6786![]() |
53.7357![]() |
K | (m s−1) | 2.20![]() |
3.44![]() |
e | 0.12![]() |
0.07![]() |
|
ω | (deg) | −91.04![]() |
−17.34![]() |
TP | (d) | 55492.0549![]() |
55528.4064![]() |
TC | (d) | 55480.7554![]() |
55543.5822![]() |
Ar | (AU) | 0.1455![]() |
0.2586![]() |
M. sini | (MJup) | 0.0259![]() |
0.0547![]() |
M. sini | (MEarth) | 8.23![]() |
17.37![]() |
γHARPS | (m s−1) | 39768.8113![]() |
|
σ(O−C) | (m s−1) | 2.05 | |
log(Post) | −440.9160![]() |
Notes. For each parameter, the median of the posterior is considered, with error bars computed from the MCMC chains using a 68.3 % confidence interval. σO−C corresponds to the weighted standard deviation of the residuals around this best solutions. All the parameters probe by the MCMC can be found in Table B.4.
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