Table E.1.
Abundances of Gaia BH3 from UVES spectrum.
| Ion | Nlines | A(X) | [X/H] | σA(X) | NLTE | |
|---|---|---|---|---|---|---|
| (1) | (2) | corr. | ||||
| C I | ... | 6.11 | -2.39 | 0.10 | 0.17 | ... |
| Mg I | 5 | 5.46 | -2.08 | 0.05 | 0.04 | 0.06a |
| Ca I | 20 | 4.13 | -2.20 | 0.10 | 0.05 | 0.14b |
| Sc II | 6 | 0.76 | -2.34 | 0.11 | 0.03 | ... |
| Ti I | 17 | 2.67 | -2.23 | 0.06 | 0.11 | ... |
| Ti II | 26 | 2.80 | -2.10 | 0.08 | 0.04 | ... |
| V I | 3 | 1.34 | -2.66 | 0.13 | 0.10 | ... |
| V II | 6 | 1.61 | -2.39 | 0.07 | 0.03 | ... |
| Cr I | 5 | 2.86 | -2.78 | 0.01 | 0.08 | ... |
| Cr II | 3 | 3.23 | -2.41 | 0.06 | 0.03 | ... |
| Mn I | 7 | 2.45 | -2.92 | 0.04 | 0.04 | ... |
| Mn II | 1 | 2.79 | -2.58 | ... | 0.08 | ... |
| Fe I | 223 | 4.96 | -2.56 | 0.12 | 0.08 | 0.10c |
| Fe II | 15 | 5.03 | -2.49 | 0.13 | 0.01 | ... |
| Co I | 7 | 2.62 | -2.30 | 0.09 | 0.11 | ... |
| Ni I | 18 | 3.68 | -2.55 | 0.12 | 0.06 | ... |
| Zn I | 1 | 2.22 | -2.40 | ... | 0.02 | 0.12d |
| Sr II | 2 | 0.50 | -2.42 | 0.05 | 0.08 | ... |
| Y II | 10 | -0.44 | -2.65 | 0.16 | 0.05 | ... |
| Zr II | 6 | 0.34 | -2.28 | 0.12 | 0.05 | ... |
| Ba II | 4 | -0.28 | -2.45 | 0.13 | 0.06 | -0.10e |
| La II | 4 | -1.22 | -2.36 | 0.07 | 0.05 | ... |
| Eu II | 1 | -1.45 | -1.97 | ... | 0.05 | ... |
a
Notes. The values A(X) are expressed in the form A(X) = log(X/H) + 12, while [X/H]=log(A(X)/A(X)⊙). The uncertainties on the abundances (σA(X)) are reported as (1) line-to-line dispersion or (2) effect of Teff uncertainty. NLTE corrections are from Bergemann et al. (2017)
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