Table 9: Iron abundances for stars observed with UVES.
Star Fe I Fe II

n [Fe/H] rms n [Fe/H] rms

25072 26 -1.46 0.10 1 -1.59

26529 26 -1.50 0.08 3 -1.53 0.05

30409 25 -1.51 0.10 2 -1.59 0.09

30426 25 -1.46 0.11 2 -1.51 0.04

34854 23 -1.54 0.15 1 -1.56

37999 31 -1.45 0.08 3 -1.53 0.05

39672 16 -1.43 0.24

$\langle{\rm [Fe/H] I}\rangle = -1.48 \pm 0.01$

$\langle{\rm [Fe/H]II}\rangle = -1.55 \pm 0.02$

**Table 9:** Iron abundances for stars observed with UVES.
Star		Fe I			Fe II
	n	[Fe/H]	rms	n	[Fe/H]	rms
25072	26	-1.46	0.10	1	-1.59
26529	26	-1.50	0.08	3	-1.53	0.05
30409	25	-1.51	0.10	2	-1.59	0.09
30426	25	-1.46	0.11	2	-1.51	0.04
34854	23	-1.54	0.15	1	-1.56
37999	31	-1.45	0.08	3	-1.53	0.05
39672	16	-1.43	0.24
$\langle{\rm [Fe/H] I}\rangle = -1.48 \pm 0.01$
$\langle{\rm [Fe/H]II}\rangle = -1.55 \pm 0.02$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations
	3 Reddening estimates from GIRAFFE spectra
	4 Photometry and reddening
	5 Metallicity from UVES spectra
	6 Conclusions
	References