Table 1: Derived orbital parameters for HD 4208b and HD 70642b from synthetic 1-planet Kepler fits to observed radial velocity data.
Orbital parameters HD 70642b HD 4208b
$a~\textnormal{[AU]}$ $3.3 \pm 0.4$ $1.68 \pm 0.05$
e $0.1 \pm 0.06$ $0.04 \pm 0.12$
$\omega~[^{\circ}]$ $277 \pm 75$ $301 \pm 84$
$m_{\rm pl}\sin i~[M_{\rm Jup}]$ 2.0 0.80
$P~[\textnormal{days}]$ $2231 \pm 400$ $829 \pm 36$
K [m s-1] $32 \pm 5$ $18.3 \pm 2$
$T_{\rm p}~\textnormal{[JD-2~451~000 ]}$ $749 \pm 300$ $774 \pm 197$
Note: the auxiliary orbital mean anomaly is derived from the mean motion $n = 2\pi/P$ and $T_{\rm p}$. The derived minium mass is $m_{\rm pl}\sin i$, with i beeing the undetermined line-of-sight inclination.

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