All Tables

Table 1: The collected spectra for each stellar target, giving the corresponding spectrograph, the resolving power, the Julian date (HJD) and signal-to-noise ratio ( S/N) for each observation. The S/N for ÉLODIE spectra is estimated at 5550 Å. Values of $v~\sin{i}$ are from Royer et al. (2002) and given in km s^-1.
Table 2: Measured values of Fourier transform zeros and calculated parameters $v~\sin{i}$ , v and i. For $v~\sin{i}$ formal and estimated systematic errors are given. For $1\sigma$ and $2\sigma$ confidence levels in v and i, signal-to-noise ratios of the broadening function of 1000 and 500 are adopted, respectively.