All Tables

Table 1: Log of the high-resolution spectra that we discuss in this paper, obtained with the FIES spectrograph at the NOT. Dates are for start of night. HJD is given in seconds with respect to 2453952.0.
Table 2: Elemental abundances of Balloon 090100001. Average values with standard deviations are given, if more than one line was fitted. Single line measurements are given without errors. Upper limits are only given, if they constrain the abundances in a reasonable way. $\log~\epsilon=12-\log(n(M)/n(H))$ . [M/H] abundances relative to solar values are taken from Grevesse & Sauval (1998). The abundances of the comparison star Feige 48 are derived from optical spectra using mostly the same line data as well as line lists, and are taken from Heber et al. (2000).
Table 3: Number of narrow spectral lines used for the cross-correlation analysis.
Table 4: Results of fits to the CCF profile variations. Listed are the best fits, with reduced $\chi ^2$ within $[\chi ^2_{\rm min}, \chi ^2_{\rm min}+1]$ , and below the separation the best fits for every ( $\ell =2$ , $\vert m\vert \le \ell$ ) combination. Inclination angle is given in degrees, the velocity amplitudes $V_{\rm p}$ and $A_{\rm M_1}$ in km s^-1, and the line-broadening $\sigma _{\rm G}$ in km s^-1.