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Table 2.
Informations on giants stars in three other samples used in this study.
| Name | Teff | πGaia | e(πGaia) | log(L/L⊙) | e(L) | Mass | e(M[−1σ]) | e(M[+1σ]) |
|---|---|---|---|---|---|---|---|---|
| Luck & Heiter (2007) | ||||||||
| 448 | 4840 | 10.9923 | 0.1299 | 1.74 | 0.03 | 2.49 | 1.1 | 0.5 |
| 3411 | 4657 | 8.7765 | 0.0385 | 1.71 | 0.02 | 2.49 | 1.28 | 0.5 |
| 3546 | 5102 | 19.4949 | 0.2307 | 1.71 | 0.03 | 2.0 | 1.09 | 0.5 |
| 4732 | 5021 | 18.2248 | 0.0565 | 1.13 | 0.02 | 1.9 | 0.3 | 0.1 |
| 5722 | 4995 | 9.7623 | 0.112 | 1.80 | 0.03 | 2.49 | 0.84 | 0.5 |
| 6037 | 4669 | 10.688 | 0.044 | 1.42 | 0.02 | 1.59 | 0.6 | 0.9 |
| 6186 | 4955 | 17.2961 | 0.3842 | 1.87 | 0.04 | 2.49 | 0.95 | 0.5 |
| 6559 | 4773 | 8.8661 | 0.0578 | 1.70 | 0.02 | 2.0 | 1.15 | 0.99 |
| 7106 | 4748 | 19.2161 | 0.2278 | 1.71 | 0.03 | 1.9 | 0.9 | 1.09 |
| 7578 | 4715 | 9.3814 | 0.0538 | 1.70 | 0.02 | 2.49 | 1.4 | 0.5 |
| 8512 | 4771 | 28.6441 | 0.413 | 1.72 | 0.03 | 1.79 | 0.94 | 1.19 |
| ... | ... | ... | ... | ... | ... | ... | ... | ... |
| Liu et al. (2014) | ||||||||
| 87 | 5072 | 8.214 | 0.1339 | 1.97 | 0.03 | 2.99 | 0.5 | 0.01 |
| 360 | 4850 | 8.9376 | 0.0836 | 1.74 | 0.03 | 2.48 | 1.5 | 0.51 |
| 448 | 4780 | 10.9923 | 0.1299 | 1.75 | 0.03 | 2.48 | 1.46 | 0.51 |
| 587 | 4893 | 17.3901 | 0.1339 | 1.21 | 0.02 | 1.7 | 0.5 | 0.3 |
| 645 | 4880 | 13.881 | 0.0803 | 1.41 | 0.02 | 2.0 | 0.5 | 0.5 |
| 1239 | 5114 | 4.7303 | 0.0955 | 2.36 | 0.03 | 3.98 | 1.0 | 0.02 |
| 1367 | 4982 | 8.875 | 0.0419 | 1.65 | 0.02 | 2.49 | 0.7 | 0.5 |
| 1419 | 4888 | 8.5872 | 0.1468 | 1.73 | 0.03 | 2.49 | 0.6 | 0.5 |
| 2114 | 5230 | 5.4912 | 0.0949 | 2.20 | 0.03 | 2.99 | 0.01 | 1.0 |
| 2952 | 4844 | 9.054 | 0.0535 | 1.75 | 0.02 | 2.49 | 1.39 | 0.5 |
| 3421 | 5287 | 3.5023 | 0.1105 | 2.73 | 0.04 | 3.97 | 0.01 | 0.99 |
| ... | ... | ... | ... | ... | ... | ... | ... | ... |
| GALAH Buder et al. (2018) | ||||||||
| 4634991546064263040 | 4064 | 0.255 | 0.0193 | 2.55 | 0.08 | 1.24 | 0.44 | 1.24 |
| 4644232799560251776 | 4052 | 0.2225 | 0.0243 | 2.43 | 0.11 | 1.0 | 0.23 | 0.87 |
| 4642633461114384640 | 4176 | 0.1932 | 0.0271 | 2.29 | 0.14 | 0.92 | 0.15 | 0.93 |
| 4622338434971333248 | 4388 | 0.3384 | 0.0196 | 1.93 | 0.07 | 0.98 | 0.2 | 0.55 |
| 4622323316686362752 | 4065 | 0.2681 | 0.0262 | 2.57 | 0.10 | 1.46 | 0.63 | 1.26 |
| 2956458403404947712 | 4461 | 0.1282 | 0.0167 | 2.36 | 0.13 | 1.11 | 0.34 | 1.36 |
| 4827471673666050816 | 4188 | 0.2602 | 0.0192 | 2.26 | 0.08 | 1.02 | 0.21 | 0.83 |
| 4800298412016784896 | 4291 | 0.2295 | 0.0208 | 2.19 | 0.10 | 1.65 | 0.76 | 1.34 |
| 2890175650594498048 | 4050 | 0.1305 | 0.0227 | 2.99 | 0.17 | 2.47 | 1.55 | 1.49 |
| 2890162456454924544 | 4434 | 0.1656 | 0.0271 | 2.45 | 0.16 | 2.99 | 1.29 | 1.98 |
| 2893967522602401792 | 4391 | 0.2155 | 0.0234 | 2.24 | 0.11 | 2.48 | 1.38 | 1.5 |
| ... | ... | ... | ... | ... | ... | ... | ... | ... |
Notes. We use HD number to identify stars observed by Luck & Heiter (2007) and Liu et al. (2014) while the Gaia identify is used for the GALAH sample. The full table is available at the CDS.
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