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Table 2
Percentiles of the distributions in Fig. 2, referred to the cut for θ in the range 85–89 days, compared with values found by AE16.
Jump parameter | Value | |
(This work) | (Anglada-Escudé et al. 2016) | |
|
||
h [ m s-1] | 1.91![]() |
|
λ [days] | 311![]() |
|
w | 0.34![]() |
|
θ [days] | 87.1![]() |
|
|
||
γHARPSpre−2016 [ m s-1] | 0.92 ± 0.56 | |
γHARPSPRD [ m s-1] | –0.58![]() |
|
γUVES [ m s-1] | –0.48![]() |
|
|
||
K1 [ m s-1] | 1.48![]() |
1.38 ± 0.21 |
P1 [days] | 11.1855![]() |
11.186![]() |
Tc,1 [JD-2 400 000] | 57 383.71![]() |
|
e1 | 0.17![]() |
<0.35 |
ω1 [rad] | –2.49![]() |
5.41 (unconstrained) |
|
||
dVr/ dt (·10-4) [ m s-1 day-1] | 3.2![]() |
2.3 ± 8.4 |
σjit,HARPSpre−2016 [ m s-1] | 1.11 ± 0.10 | 1.76![]() |
σjit,HARPSPRD [ m s-1] | 0.63![]() |
1.14![]() |
σjit,UVES [ m s-1] | 0.71![]() |
1.69![]() |
|
||
Minimum mass, mpsin i (M⊕)a | 1.21 ± 0.16 | 1.27![]() |
Orbital semi-major axis, a (AU)a | 0.048 ± 0.002 | 0.0485![]() |
Notes. They represent our adopted solution for the one-planet model. Our analysis makes use of 13 parameters as well as three values γs for the offsets, while AE16 employed 26 parameters.
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