Table 3
Atmospheric parameters of the targets.
| Star | Teff | log g | μt | [M/H] | [Fe/H](a) | [Fe/H](b) | [P/Fe](b) |
|---|---|---|---|---|---|---|---|
| (K) | (dex) | (km s−1) | (dex) | (dex) | (dex) | (dex) | |
| 2M00044180-0005553 | 4643 | 1.74 | 1.45 | −1.13 | −1.13 ± 0.15 | −1.03 ± 0.05 | 1.17 ± 0.13 |
| 2M13472354+2210562 | 5418 | 2.30 | 1.32 | −1.30 | −1.34 ± 0.18 | −1.21 ± 0.09 | 1.43 ± 0.01 |
| 2M18453994-3010465 | 3977 | 0.33 | 2.22 | −1.24 | −1.62 ± 0.21 | −1.22 ± 0.09 | 1.28 ± 0.13 |
| 2M22480199+1411329 | 4975 | 2.60 | 1.29 | −1.20 | −1.20 ± 0.15 | −1.10 ± 0.08 | 1.24 ± 0.13 |
Notes. Effective temperature Teff, surface gravity log g, and overall metallicity [M/H] are those provided by ASPCAP (García Pérez et al. 2016) using the APOGEE-2 spectra of DR17 (Abdurro'uf et al. 2022) for 2M00044180 and 2M22480199, and DR16 (Ahumada et al. 2020) for 2M13472354 and 2M18453994. The microturbulence µt is obtained from the Gaia-ESO microturbulence calibration (Smiljanic et al. 2014; Masseron et al. 2019). The errors of [Fe/H] and [P/Fe] correspond to the standard deviation of the line-by-line abundances. (a)This work. (b)Result from Paper I.
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