Open Access

Table A.3

Sample parameters calculated with methods other than spectroscopy. The Li abundances (A(Li)phot) are derived from our spectroscopic analysis with Teff,photo, log gtrig, and spectroscopic [Fe/H] as inputs.

Star name Teff,photo (K) log ɡtrig (dex) Massphot M A(Li)Phot (dex) A(Li)phot NLTE (dex)
IC2714No110 4841 ± 22 2.49 ± 0.04 2.51 ± 0.11 0.31 ± 0.10 0.54
IC2714No121 4535 ± 22 2.01 ± 0.06 2.50 ± 0.16 −0.19 ± 0.16 0.04
IC2714No126 4831 ± 13 2.29 ± 0.03 3.07 ± 0.09 0.95 ± 0.03 1.18
IC2714No190 4838 ± 31 2.40 ± 0.04 2.83 ± 0.11 0.66 ± 0.05 0.89
IC2714No220 4918 ± 61 2.31 ± 0.05 3.16 ± 0.08 0.88 ± 0.05 1.11

Notes. Effective temperature (Teff,photo) calculated from photometry, surface gravity (log ɡtrig) calculated from PARSEC isochrones with Teff,photo and Gaia parallaxes, stellar mass (Massphot) calculated from Teff,photo, log gtrig and spectroscopic [Fe/H], Li abundances (A(Li)phot) derived from FASMA with Teffp,photo, log ɡtrig, and spectroscopic [Fe/H] as inputs. The full table is available at the CDS.

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