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Table 8.
Dispersions and mean quoted uncertainties of the differential abundances found with the different spectra of the dwarf star Gaia DR2 3313689422030650496.
| Element | Abundance | Mean |
|---|---|---|
| dispersion | uncertainty | |
| Na I | 0.016 | 0.019 |
| Mg I | 0.015 | 0.007 |
| Al I | 0.015 | 0.010 |
| Si I | 0.008 | 0.027 |
| Ca I | 0.013 | 0.025 |
| Sc II | 0.023 | 0.018 |
| Ti I | 0.017 | 0.028 |
| Ti II | 0.018 | 0.034 |
| V I | 0.015 | 0.041 |
| Cr I | 0.009 | 0.039 |
| Mn I | 0.025 | 0.020 |
| Fe I | 0.011 | 0.033 |
| Fe II | 0.022 | 0.049 |
| Co I | 0.013 | 0.032 |
| Ni I | 0.007 | 0.037 |
| Cu I | 0.026 | 0.008 |
| Y II | 0.032 | 0.021 |
| Ba II | 0.023 | 0.029 |
| Ce II | 0.057 | – |
| Eu II | 0.076 | – |
Notes. For elements without an uncertainty, the abundance comes from a single line. No La II and Nd II abundances are computed for this star.
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