Table A.1.
Atmospheric parameters and abundances of LS V+22 25.
| Teff | log(g) | v sin(i) | ξ | log(n(x)) | |||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (K) | (cgs) | (km s−1) | He | C | N | O | Ne | Mg | Al | Si | S | Ar | Fe | ||
| Value | 12 720 | 3.00 | 8.7 | 0.0 | −0.50 | −4.86 | −3.38 | −4.05 | −3.67 | −5.29 | −5.96 | −4.65 | −5.15 | −5.65 | −4.50 |
| Stat. |  |
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| Sys. |  |
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| Value | 12 720 | 3.00 | 8.7 | 0.0 | −0.190 | −4.08 | −2.53 | −3.15 | −2.67 | −4.20 | −4.82 | −3.50 | −3.94 | −4.34 | −3.05 |
| Stat. |  |
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| Sys. |  |
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Notes. The abundance n(x) is either given as a fractional particle number (upper three rows) or a mass fraction (lower three rows) of species x with respect to all elements. Statistical uncertainties (“Stat.”) are 1σ confidence limits based on χ2 statistics. Systematic uncertainties (“Sys.”) cover only the effects induced by additional variations of 2% in Teff and 0.08 in log(g) and are formally taken to be 1σ confidence limits (see Irrgang et al. 2014 for details).
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