Table A.1.
Sample S2 of Li-rich K giants collected from Bharat Kumar et al. (2015) and Charbonnel et al. (2020).
| Name | V − I | G | GRVS | ϵRV |
σRV | NRV | |
|---|---|---|---|---|---|---|---|
| NRV = 8 | NRV = 40 | ||||||
| (km s−1) | (km s−1) | (km s−1) | |||||
| HD 3750 | 1.06 | 5.68 | 4.71 | 0.26 | 0.13 | 0.12 | 40 |
| HD 4042 | 0.92 | 6.51 | 5.65 | 0.25 | 0.12 | 0.13 | 19 |
| HD 5395 | 1.01 | 4.28 | 3.35 | 0.35 | 0.17 | 0.42 | 12 |
| HD 6665 * | 1.15 | 8.06 | 7.03 | 0.27 | 0.13 | 0.19 | 7 |
| HD 8676 | 1.02 | 7.48 | 6.54 | 0.26 | 0.13 | 0.13 | 45 |
| HD 9746 * | 1.20 | 5.46 | 4.39 | 0.28 | 0.14 | 0.14 | 16 |
| HD 10437 | 1.04 | 6.26 | 5.31 | 0.25 | 0.13 | 0.12 | 38 |
| HD 12203 | 0.98 | 6.47 | 5.56 | 0.25 | 0.12 | 0.13 | 11 |
| HD 19745 | 8.78 | 7.78 | 0.29 | 0.15 | 0.19 | 10 | |
| HD 30197 | 1.10 | 5.62 | 4.63 | 0.27 | 0.13 | 1.79 | 17 |
| HD 37719 | 1.04 | 7.33 | 6.38 | 0.25 | 0.13 | 0.16 | 12 |
| HD 40168 | 0.99 | 6.58 | 5.66 | 0.25 | 0.12 | 0.20 | 12 |
| HD 40827 * | 1.08 | 6.02 | 5.04 | 0.26 | 0.13 | 0.18 | 15 |
| HD 51367 | 1.11 | 6.67 | 5.67 | 0.25 | 0.12 | 0.15 | 13 |
| HD 63798 * | 0.93 | 6.23 | 5.37 | 0.25 | 0.13 | 0.15 | 19 |
| HD 233517 * | 9.27 | 8.27 | 0.31 | 0.16 | 1.53 | 3 | |
| HD 77361 | 1.08 | 5.88 | 4.90 | 0.26 | 0.13 | 0.12 | 20 |
| HD 83506 | 1.00 | 4.84 | 3.92 | 0.31 | 0.15 | 0.21 | 16 |
| HD 85563 | 1.12 | 5.25 | 4.24 | 0.29 | 0.14 | 1.99 | 22 |
| HD 88476 | 0.93 | 6.61 | 5.74 | 0.25 | 0.12 | 0.15 | 8 |
| HD 90507 | 0.92 | 6.50 | 5.64 | 0.25 | 0.12 | 0.14 | 12 |
| HD 90633 * | 1.10 | 6.00 | 5.01 | 0.26 | 0.13 | 0.13 | 17 |
| HD 93859 | 1.10 | 5.31 | 4.32 | 0.28 | 0.14 | 0.14 | 11 |
| HD 102845 | 0.94 | 5.87 | 4.99 | 0.26 | 0.13 | 0.14 | 21 |
| HD 106574 | 1.14 | 5.33 | 4.31 | 0.28 | 0.14 | 0.15 | 14 |
| HD 107484 | 1.12 | 7.39 | 6.38 | 0.25 | 0.13 | 0.15 | 17 |
| HD 108471 | 0.93 | 6.10 | 5.24 | 0.25 | 0.13 | 0.16 | 18 |
| HD 112127 * | 1.15 | 6.53 | 5.50 | 0.25 | 0.12 | 0.14 | 24 |
| HD 113049 | 1.00 | 5.70 | 4.79 | 0.26 | 0.13 | 0.49 | 22 |
| HD 115299 | 1.08 | 7.21 | 6.23 | 0.25 | 0.13 | 0.24 | 11 |
| HD 116292 * | 0.97 | 5.05 | 4.15 | 0.29 | 0.15 | 0.14 | 11 |
| IRAS 13313−5838 | 12.34 | 11.34 | 1.49 | 0.75 | 0.75 | 21 | |
| HD 118319 | 1.00 | 6.18 | 5.26 | 0.25 | 0.13 | 0.12 | 4 |
| HD 120602 | 0.90 | 5.77 | 4.93 | 0.26 | 0.13 | 0.13 | 8 |
| IRAS 13539−4153 | 12.16 | 11.16 | 1.31 | 0.66 | 0.50 | 7 | |
| HD 133086 | 0.97 | 6.56 | 5.66 | 0.25 | 0.12 | 0.14 | 13 |
| HD 145457 | 1.01 | 6.28 | 5.35 | 0.25 | 0.13 | 0.13 | 24 |
| HD 148293 | 1.08 | 4.92 | 3.94 | 0.30 | 0.15 | 0.13 | 10 |
| HD 150902 | 1.04 | 7.63 | 6.68 | 0.26 | 0.13 | 0.14 | 14 |
| HD 160781 | 1.23 | 5.54 | 4.45 | 0.28 | 0.14 | 0.14 | 12 |
| IRAS 17596−3952 | 11.80 | 10.80 | 1.01 | 0.51 | 2.70 | 3 | |
| HD 167304 | 1.01 | 6.07 | 5.14 | 0.25 | 0.13 | 0.14 | 13 |
| HD 170527 | 0.97 | 6.72 | 5.82 | 0.25 | 0.12 | 0.32 | 12 |
| TYC 3105−00152−1 | 9.53 | 8.53 | 0.33 | 0.17 | 0.23 | 3 | |
| HD 183492 | 1.02 | 5.26 | 4.32 | 0.28 | 0.14 | 0.17 | 14 |
| V859 Aql | 9.78 | 8.78 | 0.35 | 0.18 | 0.19 | 10 | |
| HD 186815 | 0.89 | 6.03 | 5.20 | 0.25 | 0.13 | 0.15 | 11 |
| HD 194937 | 1.04 | 5.92 | 4.97 | 0.26 | 0.13 | 0.15 | 18 |
| HD 196857 | 0.98 | 5.50 | 4.59 | 0.27 | 0.13 | 0.15 | 13 |
| HD 199437 | 1.11 | 4.98 | 3.98 | 0.30 | 0.15 | 0.15 | 13 |
| HD 203136 | 0.93 | 7.51 | 6.64 | 0.26 | 0.13 | 0.16 | 16 |
| HD 206078 | 0.95 | 6.85 | 5.97 | 0.25 | 0.12 | 0.13 | 15 |
| HD 212430 | 0.95 | 5.49 | 4.61 | 0.27 | 0.13 | 0.15 | 5 |
| HD 214995 | 1.08 | 5.58 | 4.60 | 0.27 | 0.13 | 0.23 | 6 |
| HD 217352 | 1.11 | 6.76 | 5.76 | 0.25 | 0.12 | 0.78 | 7 |
| HD 219025 | 1.17 | 7.33 | 6.29 | 0.25 | 0.13 | 0.30 | 16 |
Notes. An asterisk in column “Name” denotes a star already present in sample S1. When V − I is not available to convert Gaia G magnitudes into GRVS magnitudes, a typical offset of 1 mag was adopted. Values of the Gaia RV standard deviation σRV in bold face correspond to stars flagged as binaries.
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