All Tables

Table 1: The 18 planet candidates with $m_{\rm 2}\sin i <11~ M_{\rm Jup}$ detected with ELODIE at Haute-Provence Observatory.
Table 2: Observed and inferred stellar parameters for the six stars.
Table 3: Fitted orbital elements to the radial-velocity measurements for the six stars, characteristics of their planet candidate companions and properties of the fit. When necessary, we replaced the fit error by the confidence interval value issued from Monte-Carlo simulations (see text). The $m_{\rm 2} \sin i$ value is based on the $M_{\ast }$ listed in Table 2. $N_{\rm meas}$ is the number of measurements that are effectively used in the orbital solution fit. $\langle\epsilon_{\rm RV}\rangle$ is the mean measurement error and $\sigma ({\rm O-C})$ is the weighted rms of the residual. Comparison of the two values gives an indication of the amount of "jitter'' which can also be appreciated from the $\chi ^{2}_{\rm red}$ value (the reduced $\chi ^{2}$ equal to $\chi ^{\rm 2}/\nu$ where $\nu$ is the number of degrees of freedom).