Table 12: Average value of A(Li) $_{\rm NLTE}$ , average and standard deviation, and rms for the dwarf stars : mean $^{\pm {\rm aver}}_{\pm {\rm stand}}$ (rms). We separate the clean and the complete sample and give the results for 2 limits in effective temperature.
[Fe/H] ${T}_{\rm eff}$ $\geq$ 5700 K

clean complete

$\leq$ -2.5 $2.183^{\pm 0.070}_{\pm 0.097}$ (0.042) $2.156^{\pm 0.093}_{\pm 0.119}$ (0.052)

-2.5 to -2.0 $2.170^{\pm 0.067}_{\pm 0.087}$ (0.047) $2.187^{\pm 0.072}_{\pm 0.085}$ (0.057)

-2.0 to -1.5 $2.178^{\pm 0.088}_{\pm 0.109}$ (0.042) $2.183^{\pm 0.092}_{\pm 0.111}$ (0.067)

$\leq$ -1.5 $2.177^{\pm 0.071}_{\pm 0.098}$ (0.047) $2.177^{\pm 0.084}_{\pm 0.104}$ (0.052)

${T}_{\rm eff}$ $\geq$ 6000 K

clean complete

$\leq$ -2.5 $2.216^{\pm 0.038}_{\pm 0.047}$ (0.042) $2.212^{\pm 0.037}_{\pm 0.044}$ (0.052)

-2.5 to -2.0 $2.202^{\pm 0.079}_{\pm 0.091}$ (0.047) $2.202^{\pm 0.079}_{\pm 0.091}$ (0.047)

-2.0 to -1.5 $2.225^{\pm 0.088}_{\pm 0.108}$ (0.042) $2.236 ^{\pm 0.100}_{\pm 0.115}$ (0.067)

$\leq$ -1.5 $2.215^{\pm 0.074}_{\pm 0.088}$ (0.047) $2.200^{\pm 0.074}_{\pm 0.088}$ (0.052)

**Table 12:** Average value of A(Li) $_{\rm NLTE}$ , average and standard deviation, and rms for the dwarf stars : mean $^{\pm {\rm aver}}_{\pm {\rm stand}}$ (rms). We separate the *clean* and the *complete* sample and give the results for 2 limits in effective temperature.
[Fe/H]	${T}_{\rm eff}$ $\geq$ 5700 K
	clean	complete
$\leq$ -2.5	$2.183^{\pm 0.070}_{\pm 0.097}$ (0.042)	$2.156^{\pm 0.093}_{\pm 0.119}$ (0.052)
-2.5 to -2.0	$2.170^{\pm 0.067}_{\pm 0.087}$ (0.047)	$2.187^{\pm 0.072}_{\pm 0.085}$ (0.057)
-2.0 to -1.5	$2.178^{\pm 0.088}_{\pm 0.109}$ (0.042)	$2.183^{\pm 0.092}_{\pm 0.111}$ (0.067)
$\leq$ -1.5	$2.177^{\pm 0.071}_{\pm 0.098}$ (0.047)	$2.177^{\pm 0.084}_{\pm 0.104}$ (0.052)
	${T}_{\rm eff}$ $\geq$ 6000 K
	clean	complete
$\leq$ -2.5	$2.216^{\pm 0.038}_{\pm 0.047}$ (0.042)	$2.212^{\pm 0.037}_{\pm 0.044}$ (0.052)
-2.5 to -2.0	$2.202^{\pm 0.079}_{\pm 0.091}$ (0.047)	$2.202^{\pm 0.079}_{\pm 0.091}$ (0.047)
-2.0 to -1.5	$2.225^{\pm 0.088}_{\pm 0.108}$ (0.042)	$2.236 ^{\pm 0.100}_{\pm 0.115}$ (0.067)
$\leq$ -1.5	$2.215^{\pm 0.074}_{\pm 0.088}$ (0.047)	$2.200^{\pm 0.074}_{\pm 0.088}$ (0.052)

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