Table 3
ASPCAP (noncallibrated) spectroscopic parameters for the stars from APOGEE, and from DGC23: (González-Díaz et al. 2023, hereafter DGD23) in the H-band, and spectroscopic parameters from UVES from B16: Barbuy et al. (2016), B18: Barbuy et al. (2018a), B14: Barbuy et al. (2014), S21: Souza et al. (2021), L07: Lecureur et al. (2007) in the optical.
APOGEE | UVES | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
ID | Teff (K) | log g | vt (km s−1) | [Fe/H] | Ref. | SNR | Teff (K) | log g | vt (km s−1) | [Fe/H] | Ref. | SNR |
HP1-2 | 4565 | 1.54 | 0.42 | −1.229 ± 0.017 | DR17 | 122 | 4630 | 1.70 | 1.60 | −1.00 | B06 | 70 |
N6558-283 | 4570 | 2.01 | 0.30 | −1.043 ± 0.021 | DR17 | 46 | 4800 | 2.10 | 1.00 | −1.20 | B18 | 80 |
N6658-1160 | 4454 | 1.94 | 0.20 | −1.178 ± 0.019 | DR17 | 80 | 4900 | 2.60 | 1.30 | −1.15 | B18 | 80 |
N6558-1160 | 4729 | 1.80 | 1.61 | −1.15 ± 0.008 | DGD23 | – | – | – | – | – | – | – |
N6522-402361 | 4993 | 2.43 | −0.11 | −1.131 ± 0.022 | DR17 | 64 | 4990 | 2.00 | 1.40 | −1.12 | B14 | 110 |
N6522-402361 | – | – | – | – | – | – | 4990 | 2.10 | 1.40 | –1.11 | B09-G | – |
N6522-402361 | – | – | – | – | – | – | 4950 | 2.00 | 1.40 | −1.06 | Z08-G | – |
Pal6-401a | 4294 | 1.62 | 0.24 | −0.911 ± 0.018 | DR17 | 61 | 4500 | 1.50 | 1.0 | −1.00 | S21 | 50 |
Pal6-401b | 4396 | 1.80 | 0.24 | −0.911 ± 0.018 | DR17 | 105 | – | – | – | – | – | – |
OGLE-545277 | 3955 | 2.23 | 0.06 | 0.540 ± 0.010 | DR17 | 58 | 4300 | 1.40 | 1.4 | 0.07 | L07 | 60 |
OGLE-545277 | – | – | – | – | – | – | 4100 | 1.84 | 1.2 | 0.35 | Z08-G | – |
OGLE-82760 | 3967 | 2.02 | 0.10 | 0.317 ± 0.010 | DR17 | 87 | 4000 | 1.60 | 1.2 | 0.17 | L07 | 60 |
OGLE-82760 | – | – | – | – | – | – | 4300 | 1.87 | 1.5 | 0.25 | Z08-G | – |
OGLE-392918 | 4135 | 1.76 | 0.19 | −0.260 ± 0.013 | DR17 | 69 | 4100 | 1.70 | 1.5 | −0.21 | L07 | 60 |
OGLE-392918 | – | – | – | – | – | – | 4600 | 1.97 | 1.4 | 0.05 | Z08-G | – |
Notes. Parameters obtained from lower resolution FLAMES-GIRAFFE spectra from B09: Barbuy et al. (2009) and Z08: Zoccali et al. (2008), indicated by -G, are also reported.
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