Table 5: Spectrum with T=5800 K, log g = 4.25, [Fe/H]=-1.5, [S/H]=-1.10. Each Monte Carlo simulation has 500 events.
T log g [Fe/H] $\xi$ A(S) $\sigma_{\rm ran}$ $\sigma_{\rm sys}$

K cgs

5600 4.25 -1.5 1.00 6.28 0.10 +0.17

5700 4.25 -1.5 1.00 6.17 0.10 +0.06

5900 4.25 -1.5 1.00 6.05 0.11 -0.06

6000 4.25 -1.5 1.00 6.00 0.11 -0.11

5800 4.00 -1.5 1.00 6.03 0.10 -0.08

5800 4.50 -1.5 1.00 6.18 0.10 +0.07

5800 4.25 -1.0 1.00 6.34 0.10 +0.23

5800 4.25 -1.3 1.00 6.14 0.08 +0.03

5800 4.25 -1.4 1.00 6.12 0.09 +0.01

5800 4.25 -1.6 1.00 6.10 0.09 -0.02

5800 4.25 -1.7 1.00 6.08 0.10 -0.03

5800 4.25 -2.0 1.00 6.01 0.14 -0.10

5800 4.25 -1.5 1.50 6.18 0.14 +0.07

**Table 5:** Spectrum with T=5800 K, log g = 4.25, [Fe/H]=-1.5, [S/H]=-1.10. Each Monte Carlo simulation has 500 events.
T	log g	[Fe/H]	$\xi$	A(S)	$\sigma_{\rm ran}$	$\sigma_{\rm sys}$
K	cgs
5600	4.25	-1.5	1.00	6.28	0.10	+0.17
5700	4.25	-1.5	1.00	6.17	0.10	+0.06
5900	4.25	-1.5	1.00	6.05	0.11	-0.06
6000	4.25	-1.5	1.00	6.00	0.11	-0.11
5800	4.00	-1.5	1.00	6.03	0.10	-0.08
5800	4.50	-1.5	1.00	6.18	0.10	+0.07
5800	4.25	-1.0	1.00	6.34	0.10	+0.23
5800	4.25	-1.3	1.00	6.14	0.08	+0.03
5800	4.25	-1.4	1.00	6.12	0.09	+0.01
5800	4.25	-1.6	1.00	6.10	0.09	-0.02
5800	4.25	-1.7	1.00	6.08	0.10	-0.03
5800	4.25	-2.0	1.00	6.01	0.14	-0.10
5800	4.25	-1.5	1.50	6.18	0.14	+0.07

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observational data
	3 Atmospheric parameters
	4 The S I spectrum
	5 Analysis
	6 Errors and sensitivity of abundances to stellar parameters
	7 Sulphur abundances
	8 Results
	9 Discussion
	10 Conclusions
	References
	Online Material
	Appendix A: Remarks on individual stars