Astronomy & Astrophysics

Table 1: List of datasets included in the catalogue with the number of stars in the chosen range of atmospheric parameters (see text) and the method used for the Teff determination ( $\rm ldr = line$ depth ratios): A04 = Allende Prieto et al. (2004), $\rm B03=Bensby$ et al. (2003), B04a = Bensby et al. (2004a), C00 = Chen et al. (2000), E93 = Edvardsson et al. (1993), F00 = Fulbright (2000), G03 = Gratton et al. (2003), M04 = Mishenina et al. (2004), N97 = Nissen & Schuster (1997), P00 = Prochaska et al. (2000), R03 = Reddy et al. (2003).
Table 2: Statistics of the Teff comparison to Alonso et al. (1996), Blackwell & Lynas-Gray (1998) and di Benedetto (1998).
Table 3: For each element, number of stars with a determination of abundance.
Table 4: Kinematical parameters of the three considered groups and their proportion in our sample.
Table 5: Mean abundance, standard deviation and number of stars in each metallicity bin.