Table 2
Abundances for individual elements sorted according to their uncertainties.
| Element | N | N I | N II | Solar | [A/H] | dA |
|
|
||||||
| Fe | 861 | 753 | 108 | –4.59 | –4.99(05) | –0.40(05) |
| Ca | 55 | 42 | 13 | –5.73 | –5.88(05) | –0.15(05) |
| Ti | 162 | 23 | 139 | –7.14 | –7.42(09) | –0.28(09) |
| Cr | 149 | 71 | 78 | –6.40 | –6.60(11) | –0.20(11) |
| Mg | 32 | 25 | 7 | –4.51 | –4.89(15) | –0.38(15) |
| Ni | 80 | 74 | 6 | –5.81 | –6.05(16) | –0.24(16) |
| Sc | 24 | 0 | 24 | –8.99 | –9.17(19) | –0.18(19) |
| Mn | 42 | 35 | 7 | –6.65 | –7.07(21) | –0.42(21) |
| V | 44 | 2 | 42 | –8.04 | –8.27(23) | –0.23(23) |
| C | 14 | 14 | 0 | –3.65 | –3.83(24) | –0.18(24) |
| Y | 28 | 0 | 28 | –9.83 | –10.01(25) | –0.18(25) |
| Si | 13 | 4 | 9 | –4.53 | –4.77(31) | –0.24(31) |
| Co | 14 | 13 | 1 | –7.12 | –7.43(36) | –0.31(36) |
| Sr | 4 | 0 | 4 | –9.12 | –9.02(42) | +0.10(42) |
| Ba | 7 | 0 | 7 | –9.87 | –9.57(46) | +0.30(46) |
| Eu | 6 | 0 | 6 | –11.52 | –11.47(49) | +0.05(49) |
Notes. N is the number of lines with a line depth larger than rms. The uncertainties quoted between parentheses are given in terms of last digits. Columns 1 to 4 represent the element designation, the total number of spectral lines in the considered wavelength region, and in the first and the second ionization stage, respectively, while columns 5 to 7 list the solar composition, the individual abundances, and the deviation of those with respect to the solar values (Asplund et al. 2009).
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