Table A.1
Stellar parameters and Li abundances of 32 stars from the SAGA database that belong to the GSE. The last column reports references.
| Gaia DR3 ID | Name | Teff (K) |
log g (g cm−2) |
A(Li) (dex) |
err (dex) |
[Fe/H] (dex) |
err (dex) |
Ref. |
|---|---|---|---|---|---|---|---|---|
| 4376174445988280576 | BD+02_3375 | 6163 | 4.13 | 2.27 | 0.035 | −2.24 | — | [1] |
| 1776289248313154688 | BD+17_4708 | 6025 | 4.09 | 2.1 | 0.04 | −1.5 | 0.079 | [2] |
| 866863321051682176 | BD+24_1676 | 6387 | 3.84 | 2.27 | 0.035 | −2.54 | — | [1] |
| 4005317278538492928 | BD+26_2251 | 5875 | 4.13 | 2.55 | 0.05 | −1.0 | 0.079 | [2] |
| 1458016709798909952 | BD+34_2476 | 6416 | 3.95 | 2.3 | 0.035 | −2.07 | — | [1] |
| 761871677268717952 | BD+36_2165 | 6315 | 4.28 | 2.42 | 0.035 | −1.38 | — | [1] |
| 5762455439477309440 | BD-03_2525 | 5750 | 3.6 | 1.96 | 0.11 | −1.8 | 0.079 | [2] |
| 3202470247468181632 | BD-06_855 | 5378 | 4.43 | 0.98 | 0.04 | −0.69 | 0.05 | [2] |
| 5510893810476230144 | CD-45_3283 | 5672 | 4.88 | <0.7 | — | −0.83 | 0.05 | [2] |
| 5551565291043498496 | CD-48_2445 | 6222 | 4.25 | 2.22 | 0.01 | −1.93 | 0.05 | [3] |
| 5486881507314450816 | CD-57_1633 | 5933 | 4.3 | 2.22 | 0.05 | −0.9 | 0.05 | [2] |
| 6573170751851975936 | CS22881-039 | 5950 | 2.1 | < 0.6 | — | −2.75 | 0.19 | [4] |
| 6663163201607650688 | CS22947-187 | 5200 | 1.5 | < 0.5 | — | −2.61 | 0.09 | [5] |
| 6863245112083068032 | CS22950-173 | 6335 | 4.2 | 2.199 | 0.09 | −2.78 | 0.121 | [6] |
| 2676443097097288704 | CS22965-054 | 6245 | 4.0 | 2.161 | 0.09 | −2.9 | 0.136 | [6] |
| 2601354871056014336 | CS29512-073 | 5600 | 3.4 | 1.93 | 0.1 | −2.14 | 0.14 | [5] |
| 1001659495247619584 | G192-43 | 6298 | 4.39 | 2.35 | 0.035 | −1.39 | — | [1] |
| 1406910065012679680 | G202-65 | 6480 | 3.85 | 1.67 | 0.04 | −1.5 | 0.16 | [7] |
| 2688113962054816128 | G26-12 | 6089 | 4.04 | 2.23 | 0.05 | −2.48 | 0.08 | [2] |
| 2502689198705422848 | G75-31 | 6000 | 4.08 | 2.3 | 0.01 | −1.02 | 0.05 | [3] |
| 3246885466349457536 | HD024289 | 5700 | 3.5 | 2.19 | 0.08 | −2.22 | 0.1 | [7] |
| 615943806835727872 | HD084937 | 6375 | 4.06 | 2.25 | 0.028 | −2.0 | 0.079 | [2] |
| 2453397508316944128 | HE0134-1519 | 5500 | 3.2 | 1.27 | 0.19 | −3.98 | 0.3 | [8] |
| 4868057499705138560 | HE0440-3426 | 4800 | 1.6 | < 0.26 | — | −2.19 | 0.2 | [9] |
| 2988284007989400576 | J051727.4-134235 | 4961 | 1.93 | 0.91 | 0.1 | −2.14 | 0.01 | [10] |
| 5602882389229755776 | J070520.3-334324 | 4757 | 1.27 | 0.81 | 0.1 | −2.24 | 0.02 | [10] |
| 29184921251610880 | LAMOSTJ030209.33+135656.3 | 5206 | 2.3 | 2.34 | 0.12 | −1.74 | 0.3 | [11] |
| 577295698241539840 | SDSSJ090733+024608 | 5934 | 3.71 | 2.23 | 0.1* | −3.42 | 0.09 | [12] |
| 4715919175280799616 | CD-61_282 | 5909 | 4.59 | 2.12 | 0.05 | −1.15 | 0.05 | [2] |
| 4272653983123701120 | G21-22 | 5869 | 3.93 | 2.24 | 0.07 | −1.63 | — | [13] |
| 3510294882898890880 | HD111980 | 5850 | 3.94 | 2.31 | 0.1 | −1.1 | 0.08 | [14] |
| 3374633977170787072 | HD250792 | 5568 | 4.4 | 1.5 | 0.035 | −1.01 | — | [1] |
Notes. [1] Meléndez et al. (2010); [2] Smiljanic et al. (2009); [3] Asplund et al. (2006); [4] Hansen et al. (2011); [5] Masseron et al. (2012); [6] Sbordone et al. (2010); [7] Boesgaard (2007); [8] Hansen et al. (2014); [9] Hansen et al. (2015); [10] Sakari et al. (2018); [11] Li et al. (2018); [12] Bonifacio et al. (2012); [13] Bonifacio & Molaro (1997); [14] Tan et al. (2009); *private communication.
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