Open Access
Table B.1
Literature stellar properties of the set of sources used for validation.
| Star | SpType | Teff (K) | log(g/cms−2) | [Fe/H] | Reference |
|---|---|---|---|---|---|
| 15PEG | F Dwarf (V)* | 5728 ± 22 | 4.28 ± 0.03 | 0.13 ± 0.01 | García Pérez et al. (2021) |
| 18Sco | G Dwarf (V) ‡ | 5824 ± 30 | 4.42 ± 0.01 | 0.06 ± 0.01 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| 31AQL | G Subgiant (IV)* | 5776 ± 3 | 4.28 ± 0.01 | 0.59 ± 0.00 | García Pérez et al. (2021) |
| 61CygA | K Dwarf (V)‡ | 4398 ± 34 | 4.63 ± 0.01 | −0.32 ± 0.14 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| 61CygB | K Dwarf (V)‡ | 4174 ± 47 | 4.68 ± 0.02 | −0.59 ± 0.21 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| Arcturus | K Giant (III) ‡ | 4277 ± 23 | 1.58 ± 0.07 | −0.55 ± 0.04 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| BD+26_3578 | B Subgiant (IV) † | 6432 ± 2 | 3.75 ± 0.01 | −2.02 ± 0.02 | García Pérez et al. (2021) |
| BD-04_3208 | A Subgiant (IV) † | 6223 ± 50 | 3.66 ± 0.15 | −2.34 ± 0.05 | Soubiran et al. (2022) |
| G113−22 | G Subgiant (IV) † | 5595 ± 46 | 3.70 ± 0.37 | −1.07 ± 0.09 | Soubiran et al. (2022) |
| G165−39 | F Subdwarf (VI)* | 6333 ± 2 | 3.82 ± 0.01 | −1.90 ± 0.02 | García Pérez et al. (2021) |
| G207−5 | F Dwarf (V) † | 6003 ± 2 | 4.18 ± 0.01 | −0.30 ± 0.01 | García Pérez et al. (2021) |
| G28−43 | G Subdwarf (VI)* | 4923 ± 34 | 4.58 ± 0.07 | −1.56 ± 0.02 | Abdurro’uf et al. (2022) |
| G41−41 | A Subdwarf (VI)* | 6455 ± 6 | 4.07 ± 0.03 | −3.09 ± 0.66 | García Pérez et al. (2021) |
| G48−29 | A Subdwarf (VI)* | 6279 ± 111 | 3.99 ± 0.27 | −2.52 ± 0.24 | Soubiran et al. (2022) |
| G63−46 | F Dwarf (V)* | 5719 ± 42 | 3.89 ± 0.17 | −0.89 ± 0.07 | Soubiran et al. (2022) |
| G64−12 | F Subdwarf (VI)* | 6368 ± 40 | 4.11 ± 0.07 | −3.26 ± 0.05 | Soubiran et al. (2022) |
| G78−1 | F Dwarf (V) † | 5995 ± 3 | 4.11 ± 0.02 | −0.66 ± 0.02 | García Pérez et al. (2021) |
| G9−16 | F Dwarf (V)* | 6858 ±− | 4.28 ±− | −1.20 ±− | Pal et al. (2023) |
| Gmb1830 | G Dwarf (V) ‡ | 5235 ± 18 | 4.72 ± 0.01 | −1.20 ± 0.06 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| HD101177 | G Dwarf (V)* | 5887 ± 70 | 4.43 ± 0.07 | −0.26 ± 0.05 | Soubiran et al. (2022) |
| HD102158 | G Dwarf (V) † | 5761 ± 20 | 4.32 ± 0.04 | −0.43 ± 0.02 | Soubiran et al. (2022) |
| HD103095 | K Dwarf (V)* | 4991 ± 30 | 4.60 ± 0.05 | −1.26 ± 0.02 | Abdurro’uf et al. (2022) |
| HD104304 | G Subgiant (IV)* | 5441 ± 6 | 4.18 ± 0.01 | 0.32 ± 0.01 | García Pérez et al. (2021) |
| HD105631 | G Dwarf (V)* | 5402 ± 19 | 4.49 ± 0.04 | 0.18 ± 0.02 | Soubiran et al. (2022) |
| HD106210 | G Dwarf (V)* | 5664 ± 20 | 4.41 ± 0.05 | −0.10 ± 0.04 | Soubiran et al. (2022) |
| HD106516 | F Dwarf (V)* | 6274 ± 4 | 4.47 ± 0.03 | −0.82 ± 0.02 | García Pérez et al. (2021) |
| HD10697 | G Dwarf (V)* | 5610 ± 39 | 3.87 ± 0.03 | 0.16 ± 0.01 | Abdurro’uf et al. (2022) |
| HD10700 | G Dwarf (V)* | 5374 ± 2 | 4.35 ± 0.01 | −0.19 ± 0.01 | García Pérez et al. (2021) |
| HD107328 | K Giant (III) ‡ | 4576 ± 87 | 1.77 ± 0.22 | −0.36 ± 0.06 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| HD110897 | F Dwarf (V)* | 5872 ± 3 | 4.25 ± 0.02 | −0.62 ± 0.01 | García Pérez et al. (2021) |
| HD111395 | G Dwarf (V)* | 6279 ± 15 | 3.56 ± 0.03 | −0.09 ± 0.02 | Steinmetz et al. (2020) |
| HD113139 | F Dwarf (V)* | 6800 ±− | 4.10 ±− | −0.20 ±− | Gebran et al. (2016) |
| HD114174 | G Subgiant (IV)* | 5854 ±− | 4.53 ±− | −0.02 ±− | García Pérez et al. (2021) |
| HD122563 | K Bright Giant (II) ‡ | 4642 ± 35 | 1.32 ± 0.03 | −2.66 ± 0.05 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| HD140283 | G Subgiant (IV) ‡ | 5788 ± 45 | 3.75 ± 0.09 | −2.41 ± 0.04 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| HD144284 | F Dwarf (V)* | 6208 ± 48 | 3.79 ±− | 0.19 ±− | Luck (2017) |
| HD162003 | F Subgiant/Dwarf (IV/V)* | 6567 ± 86 | 4.06 ± 0.32 | −0.02 ± 0.11 | Stonkuté et al. (2020) |
| HD164259 | F Dwarf (V)* | 6815 ± 63 | 4.11 ± 0.02 | −0.10 ± 0.05 | Aguilera-Gómez et al. (2018) |
| HD220009 | K Giant (III) ‡ | 4227 ± 77 | 1.66 ± 0.04 | −0.71 ± 0.04 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| HD22879 | G Dwarf (V) ‡ | 5962 ± 86 | 4.28 ± 0.04 | −0.78 ± 0.03 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| HD284248 | G Subdwarf (VI)* | 6253 ± 3 | 4.04 ± 0.02 | −1.52 ± 0.03 | García Pérez et al. (2021) |
| HD84937 | F Dwarf (V) ‡ | 6484 ± 106 | 4.16 ± 0.05 | −1.97 ± 0.07 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| OMI_AQL | F Dwarf (V)* | 6249 ± 3 | 4.04 ± 0.01 | 0.28 ± 0.01 | García Pérez et al. (2021) |
| Procyon | F Subgiant (IV) ‡ | 6582 ± 5 | 3.98 ± 0.02 | −0.03 ± 0.02 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| Sun | G Dwarf (V) ‡ | 5771 ± 10 | 4.44 ± 0.01 | 0.00 ± 0.00 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| α CenA | G Dwarf (V) ‡ | 5804 ± 13 | 4.29 ± 0.01 | 0.22 ± 0.03 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| α Cet | K Bright Giant (II) ‡ | 3738 ± 170 | 0.66 ± 0.07 | −0.57 ± 0.17 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| α Tau | K Bright Giant (II) ‡ | 3921 ± 80 | 1.17 ± 0.05 | −0.24 ± 0.11 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| β Hyi | G Subgiant (IV) ‡ | 5917 ± 25 | 3.97 ± 0.04 | −0.06 ± 0.03 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| β Vir | F Dwarf (V) ‡ | 6093 ± 13 | 4.08 ± 0.02 | 0.13 ± 0.02 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| δ Eri | K Subgiant (IV) ‡ | 4954 ± 38 | 3.79 ± 0.10 | 0.04 ± 0.04 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| ε Eri | K Dwarf (V) ‡ | 5062 ± 29 | 4.60 ± 0.01 | −0.10 ± 0.03 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| ε Vir | K Giant (III) ‡ | 4950 ± 10 | 2.72 ± 0.02 | −0.03 ± 0.03 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| η Boo | F Subgiant (IV) ‡ | 6161 ± 18 | 3.82 ± 0.05 | 0.32 ± 0.04 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| μ Ara | G Dwarf (V) ‡ | 5974 ± 61 | 4.30 ± 0.03 | 0.41 ± 0.04 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| μ Cas | G Dwarf (V) ‡ | 5358 ± 31 | 4.49 ± 0.01 | −0.81 ± 0.04 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| μ Leo | K Giant (III) ‡ | 4519 ± 23 | 2.43 ± 0.06 | 0.19 ± 0.06 | Soubiran et al. (2024); Casamiquela et al. (2026) |
| τ Cet | G Dwarf (V) ‡ | 5397 ± 15 | 4.50 ± 0.01 | −0.47 ± 0.03 | Soubiran et al. (2024); Casamiquela et al. (2026) |
*From https://simbad.cds.unistra.fr/simbad/.
† Spectral type from https://simbad.cds.unistra.fr/simbad/, luminosity class estimated based on log (g).
‡ From https://www.blancocuaresma.com/s/benchmarkstars, i.e. Soubiran et al. (2024); Casamiquela et al. (2026).
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