Fig. 2
Comparison of our measurement of the Li equivalent width obtained with a Gaussian fit and similar measurements obtained by other authors for the same stars (Christian & Mathioudakis 2002; Wichmann et al. 2000; Gregorio-Hetem & Hetem 2002; de Laverny et al. 2003; Takeda & Kawanomoto 2005; Jasniewicz et al. 1999; Montes et al. 2001).
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