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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