All Tables

Table 1: Spectra obtained with the FOCES echelle spectrograph at the Calar Alto 2.2 m telescope in August 2001 (top section), and with the UVES echelle spectrograph at the ESO VLT telescope in March 2001 (bottom section). Columns are mostly self-explanatory. Parallaxes (mas), their errors $\sigma$ , and proper motions (mas/y) are taken from the H IPPARCOS catalogue (ESA 1997). N and $t_{\rm exp}$ refer to the number of spectra taken and the total exposure time (s).
Table 2: Metal lines used to determine element abundances. f values and damping constants have been determined from solar spectrum fits.
Table 3: Final stellar parameters and abundances of the program stars. For the description of stellar masses and ages see Sect. 5.
Table 4: Kinematic data of the program stars. Velocities are in km s^-1. Radial velocities are own measurements, except for binaries. LSR velocities are calculated for a solar motion of $(U,V,W)_\odot$ = (10.0, 5.2, 7.2) km s^-1. Preliminary population membership assignments in the rightmost column are for thin disk (D), thick disk (T) and halo (H). See last section for an explanation.
Table 5: Error propagation of basic stellar parameters when interpolating tracks of stellar evolution for HD 148816. Variations are given with respect to the final parameters in Table 3.