Table 16: Sample stars with published 6Li detection. The data are from Smith et al. (1998, sln98), Cayrel et al. (1999a, c99) and Nissen et al. (2000, n00). Columns 2 and 3 give the ${T}_{\rm eff}$ (2) and [Fe/H] values that we attributed to the stars while Cols. 4 and 5 display the values quoted in the original papers. For completeness, we note that a re-analysis by Asplund et al. (2005) of HIP 8572 and HIP 96115 from very high resolution and S/N UVES (Dekker et al. 1999) spectra finds a slightly less than 2$\sigma $ detection for HIP 8572 and no 6Li detection for HIP 96115.

HIP
${T}_{\rm eff}$  [Fe/H] ${T}_{\rm eff}$  [Fe/H] Li 6Li/7Li Ref
  (2)   lit lit NLTE    

8572
6287 -2.51 6295 -2.15 2.236 $0.02\pm0.01$ n00
48152 6377 -2.28 6300 -2.30 2.249 $0.05\pm0.02$ c99
      6300 -2.25   $0.06\pm0.02$ n00
96115 6322 -2.42 6280 -2.60 2.223 $0.05\pm0.03$ sln98


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