Table D.1.
Metallicity calibration stars.
| Name | Literature [Fe/H] | Source of [Fe/H] | Source of spectrum | Na EW [Å] | CO EW [Å] | Derived [Fe/H] |
|---|---|---|---|---|---|---|
| HD 6268 | −2.382 | 2 | XSL, 3 | −0.57085 | −0.0744 | −2.01341 |
| HD 16456 | −1.382 | 2 | XSL, 3 | −0.97503 | −0.11402 | −1.20498 |
| HD 139717 | 0.298 | 2 | XSL, 3 | −1.37645 | −0.11079 | −0.41259 |
| HD 178287 | 0.268 | 2 | XSL, 3 | −2.01691 | −0.14897 | 0.85605 |
| HD 53003 | 0.148 | 2 | XSL, 3 | −1.52129 | −0.3269 | −0.16019 |
| HD 105262 | −1.852 | 2 | XSL, 3 | −0.50033 | −0.35391 | −2.16084 |
| HD 179315 | 0.338 | 2 | XSL, 3 | −1.77065 | −0.51751 | 0.30245 |
| HD 161817 | −1.222 | 2 | XSL, 3 | −0.79191 | −0.54579 | −1.60488 |
| HD 166161 | −1.122 | 2 | XSL, 3 | −0.85418 | −0.84563 | −1.50597 |
| HD 48616 | 0.168 | 2 | XSL, 3 | −1.19382 | −0.90589 | −0.86107 |
| HD 2796 | −2.442 | 2 | XSL, 3 | −0.6748 | −0.93804 | −1.85334 |
| HD 17072 | −1.002 | 2 | XSL, 3 | −0.88558 | −1.17352 | −1.44881 |
| HD 85773 | −2.262 | 2 | XSL, 3 | −0.59183 | −1.19293 | −2.01239 |
| HD 172365 | 0.208 | 2 | XSL, 3 | −1.56569 | −1.2126 | −0.17291 |
| HD 186478 | −2.222 | 2 | XSL, 3 | −0.8696 | −1.31837 | −1.49354 |
| HD 204543 | −1.972 | 2 | XSL, 3 | −0.64096 | −1.38151 | −1.92396 |
| NGC 6397 211 | −1.972 | 2 | XSL, 3 | −0.8847 | −1.38269 | −1.47791 |
| BD+18 2890 | −1.472 | 2 | XSL, 3 | −0.9283 | −1.38975 | −1.38489 |
| HD 165195 | −2.182 | 2 | XSL, 3 | −0.17826 | −1.47843 | −2.77524 |
| NGC 7078 1079 | −2.33466 | 1 | XSL, 3 | −0.63271 | −1.53196 | −1.94662 |
| HD 9051 | −1.607 | 2 | XSL, 3 | −1.05279 | −1.84992 | −1.19017 |
| 2MASS J18352834−3444085 | −1.507 | 2 | XSL, 3 | −1.04436 | −1.91434 | −1.21294 |
Notes. The full table is only available at the CDS. Column 1 lists the name, Col. 2 the metallicity from the literature source (given in 3); Col. 4 the source of the K-band spectrum; Cols. 5 and 6 give the line indices of Na and CO used for the metallicity determination; Col. 7 gives the derived metallicity determined by us.
References. (1) Ahumada et al. (2020); (2) Arentsen et al. (2019); (3) Gonneau et al. (2020); (4) Magrini et al. (2010); (5) Thorsbro et al. (2020).
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