Table 1
Preliminary parameters from the literature.
Name | Teff (K) | log ɡ | [Fe/H] | θ (mas) | Ref(Teff/log ɡ/[Fe/H]/θ) | Inst. | E(B – V) |
---|---|---|---|---|---|---|---|
Giants with interferometric measurements | |||||||
HD 2665 | 4883 ± 95 | 2.21 ± 0.03 | −2.10 ± 0.10 | 0.395 ± 0.004 | K20 | HE | 0.024 |
HD 122563 | 4635 ± 34 | 1.40 ± 0.04 | −2.75 ± 0.12 | 0.925 ± 0.011 | K20 | HE | 0.027 |
HD 175305 | 4850 ± 118 | 2.50 ± 0.03 | −1.52 ± 0.08 | 0.484 ± 0.006 | K20 | HE | 0.011 |
HD 221170 | 4248 ± 128 | 1.25 ± 0.04 | −2.40 ± 0.13 | 0.596 ± 0.005 | K20 | HE | 0.058 |
Giants with direct IRFM measurements | |||||||
HD 45282 | 5299 ± 87 | 3.16 | −1.45 | 0.270 ± 0.009 | Ca10 | UV | 0.002 |
HD 175305 | 5059 ± 80 | 2.53 ± 0.14 | −1.29 | 0.447 ± 0.006 | Hw16 | HE | 0.011 |
HD 218857 | 5162 ± 80 | 2.66 ± 0.32 | −1.78 | 0.194 ± 0.003 | Hw16 | UV | 0.018 |
BPS BS 17569–049 | 4781 | 1.20 | −2.88 | – | Ca21/Ca04/Ca04/– | UV | 0.034 |
BPS CS 22953–003 | 5200 | 2.30 | −2.84 | – | Ca21/Ca04/Ca04/– | UV | 0.015 |
BPS CS 22892–052 | 4941 | 1.60 | −3.03 | – | Ca21/Ca04/Ca04/– | UV | 0.027 |
Giants with asteroseismic measurements | |||||||
HD 3179 | 5290 ± 105 | 2.58 | −1.00 | – | Ho21/St18/PA/– | FE | 0.017 |
HD 13359 | 5322 ± 106 | 2.48 | −0.98 | – | Ho21/St18/PA/– | FE/UV | 0.014 |
HD 17072 | 5364 ± 107 | 2.61 | −0.98 | – | Ho21/St18/PA/– | UV | 0.004 |
HD 221580 | 5244 ± 104 | 2.40 | −1.20 | – | Ho21/St18/PA/– | HA | 0.009 |
TIC 168924748 | 5148 ± 102 | 2.68 | −0.61 | – | Ho21/Bu21/Ca21/– | – | 0.096 |
TIC 404605506 | 5228 ± 104 | 2.44 | −0.64 | – | Ho21/Bu21/Ca21/– | – | 0.057 |
Other giants | |||||||
HD 6229 | 5055 | 2.12 | −1.21 | – | Ar19 | UV | 0.047 |
HD 105740 | 4718 | 2.76 | −0.66 | – | Ar19 | UV | 0.022 |
HD 115444 | 4500 | 0.70 | −3.15 | – | Jh12 | HE | 0.012 |
HD 186478 | 4716 | 1.57 | −2.31 | – | Ar19 | UV | 0.150 |
BD+09 2860 | 5369 | 2.57 | −1.58 | – | Ar19 | UV | 0.025 |
BD+09 2870 | 4664 | 1.47 | −2.34 | – | Ar19 | UV | 0.025 |
BD+11 2998 | 5480 | 3.00 | −1.12 | – | Kl12 | UV | 0.031 |
BD+17 3248 | 5240 | 2.44 | −2.07 | – | Cr08 | UV | 0.051 |
BD–18 5550 | 4750 | 1.40 | −3.06 | – | Ca04 | UV | 0.172 |
CD–30 298 | 5223 | 2.92 | −3.50 | – | Be17 | UV | 0.020 |
CD–41 15048 | 5726 | 2.04 | −2.24 | – | Be17 | UV | 0.013 |
CD–62 1346 | 5163 | 1.96 | −1.54 | – | Ar19 | UV | 0.032 |
BPS CS 22186–025 | 4900 | 1.25 | −3.00 | – | Ca04 | UV | 0.025 |
BPS CS 22189–009 | 4900 | 1.70 | −3.49 | – | Ca04 | UV | 0.022 |
BPS CS 22891–209 | 4700 | 1.00 | −3.29 | – | Ca04 | UV | 0.066 |
BPS CS 22896–154 | 5250 | 2.70 | −2.69 | – | Ca04 | UV | 0.047 |
BPS CS 22897–008 | 4900 | 1.70 | −3.41 | – | Ca04 | UV | 0.014 |
BPS CS 22949–048 | 4800 | 1.50 | −3.25 | – | Sp11 | UV | 0.031 |
BPS CS 22956–050 | 4900 | 1.70 | −3.33 | – | Ca04 | UV | 0.029 |
BPS CS 22966–057 | 5300 | 2.20 | −2.62 | – | Ca04 | UV | 0.016 |
BPS CS 29491–053 | 4700 | 1.30 | −3.04 | – | Ca04 | UV | 0.017 |
BPS CS 29502–042 | 5100 | 2.50 | −3.19 | – | Ca04 | UV | 0.056 |
BPS CS 29518–051 | 5200 | 2.60 | −2.69 | – | Ca04 | UV | 0.013 |
BPS CS 30325–094 | 4950 | 2.00 | −3.30 | – | Ca04 | UV | 0.036 |
BPS CS 31082–001 | 4876 | 1.80 | −2.81 | – | Ha18 | UV | 0.014 |
CEMP giants | |||||||
HD 26 (CEMP-s) | 5169 | 2.46 | −0.98 | – | Kk21 | HE | 0.044 |
HD 5223 (CEMP-rs) | 4650 | 1.03 | −2.00 | – | Kk21 | HE | 0.037 |
HD 76396 (CEMP-rs) | 4750 | 2.00 | −2.27 | – | Kk21 | HE | 0.025 |
HD 196944 (CEMP-rs) | 5168 | 1.28 | −2.50 | – | Kk21 | HE | 0.025 |
HD 201626 (CEMP-s) | 5084 | 2.18 | −1.75 | – | Kk21 | HE | 0.056 |
HD 224959 (CEMP-rs) | 4969 | 1.26 | −2.36 | – | Kk21 | HE | 0.029 |
HE 0507-1653 (CEMP-s) | 5035 | 2.39 | −1.35 | – | Kk21 | HE | 0.048 |
Notes. The “Ref” column indicates the stellar parameter reference. The “Inst.” column specifies the origin of the spectra used in the present paper: HERMES (HE), HARPS (HA), UVES (UV) or FEROS (FE). The E(B – V) column provides reddening values extracted from Capitanio et al. (2017) when available, or alternatively from Schlafly & Finkbeiner (2011). CEMP-s and -rs are carbon-enriched metal-poor stars enriched in either s or in a mixture of s and r elements, following the classification in Karinkuzhi et al. (2021). HD 175305 is repeated twice because it has both interferometric and IRFM data.
References. K20: Karovicova et al. (2020); C10: Casagrande et al. (2010); Hw16: Hawkins et al. (2016); Ca21: Casagrande et al. (2021); Ca04: Cayrel et al. (2004); Sp11: Spite et al. (2011); Bu21: Buder et al. (2021); Ho21: Hon et al. (2021); St18: Stassun et al. (2018); Bu21: Buder et al. (2021); PA: the PASTEL catalogue Soubiran et al. (2016); Kk21 Karinkuzhi et al. (2021); Ar19: Arentsen et al. (2019); Jh12: Johnson (2002); Kl12: Koleva & Vazdekis (2012); Cr08: Carney et al. (2008); Ha18: Hansen et al. (2018); Be17: Beers et al. (2017).
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