**Table 7:** Discrepant cases in the original works of R96, R99, and BM97. Columns identified by a $\Delta$ symbol represent the difference on that given quantity ( ${T}_{\rm eff}$ , [Fe/H], EW, and lithium abundance) between R96 and BM97 (when a target has a second entry, this refers to R99 - BM97).
HIP	$\Delta$ ${T}_{\rm eff}$	$\Delta$ [Fe/H]	$\Delta EW$	$\Delta$ A(Li)	$\Delta$ A(Li) $_{\rm end}^{{a}}$
	K	dex	mÅ	dex	dex
3430	+144	-0.29	0.0	+0.09	-0.02
11952	-94	-0.11	0.0	-0.08	-0.01
12807	-207	+0.51	0.0	-0.11	-0.03
	-287	+0.58	+5.9	-0.11	-0.05
14594	-200	+0.05	0.0	-0.18	-0.04
23344	+230	-0.90	0.0	+0.15	0.01
	+130	-0.77	-1.5	+0.05	0.02
42592	-164	+0.20	0.0	-0.12	-0.01
	-186	-0.02	-2.9	-0.18	0.01
44605	-240	-0.34	0.0	-0.23	-0.05
66673	-178	-0.15	0.0	-0.10	0.03
	-248	+0.18	-5.8	-0.25	0.06
68592	-142	-0.49	0.0	-0.09	0.02
	-192	-0.72	+3.2	-0.01	0.07
78640	-179	+0.17	0.0	-0.17	-0.05
87693	-361	-0.25	0.0	-0.25	0.01
96115	-160	+0.18	0.0	-0.11	0.00
	-160	+0.04	+1.6	-0.11	-0.03
114962	-142	+0.23	0.0	-0.15	-0.06

^a $\Delta$ A(Li) $_{\rm end}$ represents the remaining discrepancy in the lithium abundance after having
taken into account the differences in ${T}_{\rm eff}$ (Col. 2), [Fe/H] (Col. 3), and EW (Col. 4).

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