We have performed the detailed analysis of 174 high-resolution spectra of FGK dwarfs obtained with the ELODIE echelle spectrograph at the Observatoire de Haute-Provence. Abundances of Fe, Si and Ni have been determined from equivalent widths under LTE approximation, whereas abundances of Mg have been determined under NLTE approximation using equivalent widths of 4 lines and profiles of 5 lines. Spatial velocities with an accuracy better than 1kms, as well as orbits, have been computed for all stars.

Cone search capability for table J/A+A/418/551/table8 (Atmospheric parameters, abundances, 3D velocities with respect to the Sun, orbital parameters, probability to belong to the thin disk and the thick disk for the program stars)