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Table 2

Calculated offsets in atmospheric parameters and Li abundances between literature data and this work plus R12.

Samplea ΔTeff (K) Δ log g Δ[Fe/H] ΔA(Li)
TW+R12 0 ± 00 0.00 ± 0.00 0.00 ± 0.00 0.00 ± 0.00 898 835
B10 40 ± 48 0.05 ± 0.06 0.03 ± 0.03 0.07 ± 0.09 69 117 117
G10 − 3 ± 69 − 0.02 ± 0.04 0.04 ± 0.04 − 0.14 ± 0.12 45 138 152
I09 26 ± 32 0.05 ± 0.05 0.02 ± 0.02 0.06 ± 0.04 11 79 80
LH06 46 ± 91 0.04 ± 0.20 0.01 ± 0.06 0.01 ± 0.11 77 165 194
T10 − 12 ± 54 − 0.03 ± 0.09 0.03 ± 0.04 − 0.03 ± 0.10 26 113 117
Gh10 30 ± 71 − 0.06 ± 0.14 − 0.00 ± 0.06 0.01 ± 0.08 38 253 262
LR04 − 83 ± 63 − 0.01 ± 0.11 − 0.02 ± 0.05 − 0.07 ± 0.08 212 415 451
DM14 7 ± 80 0.07 ± 0.09 0.01 ± 0.04 0.04 ± 0.12 35 307 326
DM15 46 ± 70 0.12 ± 0.12 0.03 ± 0.06 0.04 ± 0.10 65 778 836
G1415 42 ± 82 0.01 ± 0.04 0.02 ± 0.05 − 0.17 ± 0.07 29 66 68

Notes. (a) Samples correspond to: B10 = Baumann et al. (2010); G10 = Gonzalez et al. (2010); I09 = Israelian et al. (2009); LH06 = Luck & Heiter (2006); T10 = Takeda et al. (2010); Gh10 = Ghezzi et al. (2010); LR04 = Lambert & Reddy (2004); DM14 = Delgado Mena et al. (2014); DM15 = Delgado Mena et al. (2015); G1415 = Gonzalez (2014)+Gonzalez (2015); TW = This work (b) Number of stars in common between the sample and data from this work plus R12. (c) Number of stars from this sample used in the final catalog (after removal of possible spectroscopic binaries and stars without parallaxes). (d) Total number of stars in the original catalog, removing giants when necessary.

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