Table 2
Metallicities for the new C-19 member stars.
| Gaia ID | Teff (K) | δ(Teff) (K) | log g | δ(log g) | vt (km s−1) | MKs | δ(MKs) | [Fe/H] | [Fe/H]CaT | Member |
|---|---|---|---|---|---|---|---|---|---|---|
| 2820866973064504448 | 4539 | 41 | 0.79 | 0.10 | −5.10 | 0.22 | −3.26 | Y | ||
| 2758373652717936640 | 4762 | 56 | 1.33 | 0.13 | −3.90 | +0.31 | −3.14 | Y | ||
| 2288313499629002624† | 4740 | 52 | 1.27 | 0.12 | +2.31 | −4.03 | 0.29 | −3.37 | −3.35 | Y |
| 2606388641446500864 | 5479 | 110 | 3.13 | 0.21 | 1.31 | +0.42 | 0.51 | −3.12 | −2.93 | Y |
| 2606242131522123520 | 5260 | 110 | 2.59 | 0.30 | 1.60 | −0.90 | 0.71 | −3.07 | −3.07 | Y |
| 6600784780223506944 | 4552 | 38 | 0.83 | 0.09 | 2.46 | −5.04 | 0.21 | −3.29 | −3.42 | Y |
| 6559328209695612544 | 4668 | 51 | 1.11 | 0.12 | 2.40 | −4.40 | 0.28 | −3.25 | −3.17 | Y |
| 6594796290142997376 | 4812 | 56 | 1.45 | 0.13 | 2.22 | −3.62 | 0.31 | −3.28 | −3.29 | Y |
| 6567859904530795904 | 5289 | 81 | 2.67 | 0.22 | 1.56 | −0.70 | 0.54 | −3.30 | −3.03 | Y |
| 2641204161744171392 | 4832 | 76 | 1.49 | 0.18 | 2.20 | −3.50 | 0.43 | −3.29 | −3.39 | Y |
| 2852330082409525760 | 4957 | 80 | 1.74 | 0.26 | −2.93 | 0.63 | −3.35 | Y | ||
| 2760807387346283648 | 5232 | 88 | 2.51 | 0.24 | −1.08 | 0.58 | −3.20 | Y | ||
| 2871048855556252160 | 5260 | 93 | 2.59 | 0.25 | −0.89 | 0.61 | −2.93 | P | ||
| 2658115921889849472 | 5412 | 103 | 2.99 | 0.25 | +0.07 | 0.60 | −2.61 | P | ||
| 2644950674600720512 | 5224 | 109 | 2.49 | 0.30 | −1.12 | 0.71 | −3.27 | Y | ||
| 2640793013114783872 | 5417 | 111 | 2.99 | 0.26 | 1.39 | +0.08 | 0.62 | −2.59 | −3.02 | P |
Notes. The star with the dagger symbol has spectra from both Subaru/HDS and INT/IDS, which give [Fe/H] and [Fe/H]CaT respectively. Stars denoted by “Y” are confirmed C-19 members that have either [Fe/H] or [Fe/H]CaT within the systematic uncertainty of the C-19 stream (0.2 dex). Those denoted by “P” are probable members that have metallicities beyond the systematic uncertainty.
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