Table 3
Abundance results of J051213.81-693537.1.
| J051213 | Sun | |||||
| Teff = 5875 K | ξt = 3.0 km s-1 | |||||
| log g = 1.00 dex | [Fe/H] = −0.56 dex | |||||
|
|
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| Ion | N | log ϵ | σ l2l | [X/Fe] | σ tot | log ϵ⊙ |
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| C I | 1 | 8.75 | 0.20 | 0.88 | 0.26 | 8.43 |
| O I | 1 | 8.65 | 0.20 | 0.52 | 0.26 | 8.69 |
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| Mg I | 1 | 7.00 | 0.20 | –0.04 | 0.24 | 7.60 |
| Al I | 1 | 6.60 | 0.20 | 0.71 | 0.25 | 6.45 |
| Si I | 4 | 7.32 | 0.05 | 0.37 | 0.18 | 7.51 |
| S I | 2 | 6.51 | 0.03 | –0.05 | 0.13 | 7.12 |
| Ca I | 11 | 6.00 | 0.09 | 0.22 | 0.09 | 6.34 |
| Ca II | 1 | 6.00 | 0.20 | 0.22 | 0.24 | 6.34 |
| Sc II | 3 | 2.93 | 0.03 | 0.34 | 0.10 | 3.15 |
| Ti I | 2 | 4.69 | 0.07 | 0.30 | 0.13 | 4.95 |
| Ti II | 7 | 4.62 | 0.13 | 0.23 | 0.11 | 4.95 |
| V I | 1 | 3.91 | 0.20 | 0.54 | 0.25 | 3.93 |
| V II | 2 | 3.91 | 0.04 | 0.54 | 0.14 | 3.93 |
| Cr I | 4 | 5.20 | 0.07 | 0.12 | 0.10 | 5.64 |
| Cr II | 7 | 5.16 | 0.11 | 0.08 | 0.10 | 5.64 |
| Mn I | 1 | 4.69 | 0.20 | –0.18 | 0.24 | 5.43 |
| Fe I | 53 | 6.94 | 0.10 | 0.00 | 0.06 | 7.50 |
| Fe II | 13 | 6.94 | 0.09 | 0.00 | 0.07 | 7.50 |
| Ni I | 4 | 5.75 | 0.08 | 0.09 | 0.12 | 6.22 |
| Zn I | 1 | 4.22 | 0.20 | 0.22 | 0.29 | 4.56 |
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| Y II | 5 | 3.13 | 0.11 | 1.48 | 0.13 | 2.21 |
| Zr II | 2 | 3.20 | 0.02 | 1.18 | 0.10 | 2.58 |
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| La II | 6 | 2.52 | 0.13 | 1.98 | 0.13 | 1.10 |
| Ce II | 6 | 2.91 | 0.12 | 1.89 | 0.13 | 1.58 |
| Pr II | 6 | 1.96 | 0.06 | 1.80 | 0.13 | 0.72 |
| Nd II | 14 | 2.67 | 0.10 | 1.81 | 0.13 | 1.42 |
| Sm II | 1 | 1.70 | 0.20 | 1.30 | 0.24 | 0.96 |
| Eu II | 2 | 0.98 | 0.07 | 1.02 | 0.13 | 0.52 |
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| Dy II | 2 | 2.00 | 0.20 | 1.46 | 0.21 | 1.10 |
| Er II | 2 | 1.90 | 0.20 | 1.54 | 0.22 | 0.92 |
| Pb Iu | 1 | 3.30 | 0.20 | 2.11 | 0.25 | 1.75 |
| Th IIu | 1 | 1.35 | 0.20 | 1.89 | 0.27 | 0.02 |
Notes. The table lists for each ion the used number of lines (N) for the abundance determination, the determined abundance (log ϵ), the uncertainty of this abundance due to line-to-line scatter (σl2l), the element over iron ratio ([X/Fe]), and total uncertainty (σtot). The total uncertainty σtot includes line-to-line scatter and atmospheric parameter uncertainty (see text for details). The last column lists the solar abundances from Asplund et al. (2009). We choose a standard deviation of 0.20 dex for all ions for which the abundance was derived using spectrum synthesis or for which only one line is available.
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