Astronomy & Astrophysics

Table 1: Adopted stellar parameters ( $T_{\rm eff}$ , $\log~ g$ , and $\xi$ ) and heliocentric radial velocity ( $V_{\rm r}$ ) for the Bulge sample stars. Two quality indicators of the observed spectra are also given: the mean DAOSPEC residuals and S/N per 0.017 Å pixel around $\lambda$ 6330 Å.
Table 2: Equivalent widths of FeI lines for stars in the Blanco field. The full table is available at the CDS.
Table 3: Equivalent widths of FeI lines for stars in the b=-6 field. The full table is available at the CDS.
Table 4: Equivalent widths of FeI lines for stars in the b=-3 field. The full table is available at the CDS.
Table 5: Equivalent widths of FeI lines for RGB stars in Baade's window. The full table is available at the CDS.
Table 6: Equivalent widths of FeI lines for Red Clump stars in Baade's window. The full table is available at the CDS.
Table 7: S/N influence on spectroscopic stellar parameters determination.
Table 8: Astrophysical gf-values determined by this study compared with others values extracted from the VALD and NIST database.
Table 9: Abundances of Arcturus and $\mu$ Leo.
Table 10: Abundance uncertainties associated with the stellar parameters.
Table 11: Abundances of Fe, O, Mg, Al, Na, C, and N for the program stars. The flag column describes the quality of the O measurement: 0 = good measurement; 1 = uncertain measurement due to telluric lines in the vicinity or bad quality fit; 2 = no measurement.
Table 12: Abundances from individual Na and Al lines.