Table 2
Stellar parameters and phosphorus abundances of our programme stars and comparisons, when available, with the analysis on the CRIRES spectra from (Caffau et al. 2011).
| Target | Teff | log g | [Fe/H] | [S/H] | Ref. | EW [pm] | A(P) | EW [pm] | A(P) | ||||
| Crires | Giano | Crires | Giano | Crires | Giano | Crires | Giano | ||||||
| K | 1053.2 | 1053.2 | 1058.4 | 1058.4 | |||||||||
|
|
|||||||||||||
| HD 1461 | 5765 | 4.38 | + 0.19 | −0.05 | G10 | 2.00 | 2.10 | 5.59 | 5.62 | 2.70 | 2.70 | 5.59 | 5.59 |
| HD 10453 | 6368 | 3.96 | −0.46 | −0.29 | C02 | <3.00 | <5.28 | ||||||
| HD 13555 | 6470 | 3.90 | −0.27 | −0.25 | T02 | 1.80 | 2.34 | 5.14 | 5.28 | 2.90 | 3.13 | 5.22 | 5.27 |
| HD 22484 | 5960 | 4.02 | −0.25 | −0.28 | T02 | 1.90 | 5.33 | 3.00 | 5.41 | ||||
Reference. The column “Ref” refers to the reference for the stellar parameters and [S/H], and corresponds to G10: González Hernández et al. (2010); T02: Takada-Hidai et al. (2002); C02: Chen et al. (2002).
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