**Table 6:** Final Li abundances as derived by using different sets of ${T}_{\rm eff}$ . The whole table is available on-line.
HIP	bin	[Fe/H]	$\sigma$ (Fe)	log g	EW	$\pm$ $1\sigma$	A(Li) $_{\rm LTE}$	A(Li) $_{\rm NLTE}$	$+1\sigma$	$-1\sigma$	A(Li) $_{\rm S98}$	A(Li) $_{\rm H97}$
		dex	dex	cm s^-1	mÅ	mÅ	dex	dex	dex	dex	dex	dex
Sample #1: the clean sample
911		-1.84	0.15	4.50	30.8	3.5	2.117	2.112	0.042	0.067	2.200	2.191
3026		-1.25	0.07	3.85	45.0	6.0	2.428	2.418	0.078	0.086	2.573	2.567
3446		-3.50	0.10	4.50	27.0	3.9	1.973	1.986	0.074	0.076	2.045	2.048
3564		-1.27	0.15	3.50	35.2	3.5	2.011	2.054	0.056	0.076	2.244	2.008
8572		-2.51	0.01	3.85	27.0	1.4	2.257	2.236	0.026	0.027	2.239	2.257
...		...	...	...	...	...	...	...	...	...	...	...
Sample #2: the $\beta$ sample
484		-1.23	0.15	3.00	12.1	3.5	0.953	1.101	...	...	0.949	...
3554		-2.87	0.15	3.00	17.7	3.5	1.018	1.153	0.087	0.104	1.044	1.238
4343		-2.08	0.15	3.00	9.1	3.5	0.766	0.912	0.150	0.219	0.878	0.680
8314	?	-1.68	0.09	4.00	27.0	3.0	2.378	2.337	0.053	0.058	2.262	2.523
13 749		-1.62	0.15	3.00	14.6	3.5	0.876	1.039	0.102	0.128	0.901	0.870
...		...	...	...	...	...	...	...	...	...	...	...
Sample #3: the ubvy sample
12 807		-2.87	0.22	4.50	22.9	3.0	1.918	1.929	0.066	0.068	2.676	1.940
83 320		-2.56	0.15	3.50	<5.0	...	<1.265	<1.287	...	...	<1.603	1.167
87 062		-1.67	0.23	4.50	31.5	4.0	2.109	2.111	0.088	0.069	2.109	2.106
91 129	*	-2.96	0.10	4.50	27.3	2.5	2.208	2.191	0.045	0.054	2.899	2.224
103 337		-2.07	0.15	3.00	25.8	3.5	1.025	1.197	0.069	0.072	1.179	0.877
...		...	...	...	...	...	...	...	...	...	...	...

? Identifies a suspected binary (Latham et al. 2002; Carney et al. 1994, 2003).
* Identifies a confirmed single- or double-lined binary (from Latham et al. 2002; Carney et al. 1994, 2003).
Note that the complete version of the table (available only on-line) reports the complete legend of symbols and references.

Source LaTeX | All tables | In the text

	1 The lithium paradigm
	2 The "Lithium plateau debate''?
	3 Sample selection: a critical analysis of the literature
	4 Stellar parameters: I. Gravity, metallicity, and microturbulence
	5 Stellar parameters. II. The temperature scale and its weaknesses
	6 Our final choice: temperature and data-sample(s)
	7 The lithium abundance
	8 Preliminary results on the mean lithium abundance and the dispersion
	9 Evolutionary status of the stars
	10 The lithium abundance along the plateau for the dwarf stars
	11 The lithium abundance in evolved stars
	12 Duplicity and variability
	13 Stars with extreme Li abundances
	14 Implications for stellar structure and evolution
	15 Summary and conclusions
	References
	Online Material