All Tables

Table 1: A sample of results from the automatic analyses. We list the names, HD numbers and spectral types from the manual spectral typing. We give the $T_{\rm eff}$ , $\log g$ and [Fe/H] and estimated uncertainties determined by VASP and VWA. $v \sin i$ values are calculated with VWA and have uncertainties of 10-20%. The first four targets are not VSOP targets, but high S/N HARPS spectra taken from Dall et al. (2006), which we have used to calibrate our tools. Full detailed results for all VSOP stars can be found online (see text).
Table 2: The VSOP stars of the first observing season.