Table 9
Abundances derived from APOGEE and UVES spectra with TURBOSPECTRUM, adopting the best-suited stellar parameters, as explained in Sect. 4.1.
| Model | H-band Opt | H-band Opt | H-band Opt | H-band Opt | H-band Opt | H-band Opt | H-band Opt | H-band Opt | ||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Star | HP1-2 | 283 | 1160 | 402361 | 401 | 545277 | 82760 | 392918 | ||||||||
| C | −0.15 | – | 0.12 | – | 0.00 | – | 0.08 | – | 0.00 | – | 0.10 | – | −0.10 | – | −0.20 | – |
| N | 0.40 | – | 0.35 | – | 0.00 | – | 0.30 | – | 0.20 | – | 0.40 | – | 0.05 | – | 0.10 | – |
| O | 0.45 | – | 0.45 | – | 0.30 | – | 0.50 | – | 0.25 | – | 0.50 | – | −0.05 | – | +0.10 | – |
| Na | – | −0.20 | – | 0.50 | – | 0.25 | – | 0.08 | 0.03 | −0.10 | 0.70 | 0.80 | 0.37 | 0.40 | 0.00 | 0.35 |
| Mg | 0.21 | 0.15 | 0.24 | – | 0.25 | 0.25 | 0.30 | 0.30 | 0.24 | 0.23 | 0.00 | 0.00 | –0.15 | –0.15 | 0.10 | 0.10 |
| Al | 0.32 | 0.37 | 0.90 | 0.60 | 0.40 | – | 0.08 | 0.32 | 0.32 | 0.25 | 0.70 | 0.65 | 0.70 | 0.50 | 0.35 | 0.35 |
| Si | 0.35 | 0.30 | 0.40 | 0.45 | 0.20 | 0.40 | 0.30 | 0.00 | 0.30 | 0.46 | 0.06 | 0.00 | 0.05 | 0.05 | 0.15 | 0.15 |
| Ca | 0.12 | 0.10 | – | 0.15 | 0.20 | 0.25 | 0.22 | −0.07 | 0.26 | 0.00 | 0.35 | 0.48 | 0.05 | 0.05 | 0.15 | 0.15 |
| Ti | – | 0.22 | – | 0.20 | – | 0.15 | – | 0.25 | – | 0.15 | – | 0.40 | – | 0.30 | – | 0.00 |
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