Table 1
Initial parameters and data information for the GBS.
Star ID | [Fe/H]LIT | σ[Fe/H] | N | T eff | σ T eff | log g | σ log g | v sini | Ref v sini | Source | R (k) | S/N | Extra spectra |
|
|||||||||||||
18 Sco | 0.03 | 0.03 | 15 | 5747 | 39 | 4.43 | 0.01 | 2.2 | Saar | N | 80 | 380 | H |
61 Cyg A | –0.20 | 0.11 | 5 | 4339 | 27 | 4.43 | 0.16 | 0.0 | Benz | N | 80 | 360 | – |
61 Cyg B | –0.27 | 0.00 | 2 | 4045 | 25 | 4.53 | 0.04 | 1.7 | Benz | N | 80 | 450 | – |
α Cen A | 0.20 | 0.07 | 9 | 5840 | 69 | 4.31 | 0.02 | 1.9 | Br10 | H | 115 | 430 | U, H* |
α Cen B | 0.24 | 0.04 | 7 | 5260 | 64 | 4.54 | 0.02 | 1.0 | Br10 | H | 115 | 460 | – |
α Cet | –0.26 | 0.23 | 8 | 3796 | 65 | 0.91 | 0.08 | 3.0 | Zama | N | 80 | 300 | H, U |
α Tau | –0.23 | 0.3 | 15 | 3927 | 40 | 1.22 | 0.10 | 5.0 | Hekk | N | 80 | 320 | H |
Arcturus | –0.54 | 0.04 | 11 | 4247 | 37 | 1.59 | 0.04 | 3.8 | Hekk | N | 80 | 380 | H, U, U.P |
β Ara | 0.5 | 0.00 | 1 | 4073 | 64 | 1.01 | 0.13 | 5.4 | Me02 | H | 115 | 240 | – |
β Gem | 0.12 | 0.06 | 5 | 4858 | 60 | 2.88 | 0.05 | 2.0 | Hekk | H | 115 | 350 | – |
β Hyi | –0.11 | 0.08 | 6 | 5873 | 45 | 3.98 | 0.02 | 3.3 | Re03 | U.P | 80 | 650 | N, H, U |
β Vir | 0.13 | 0.05 | 11 | 6083 | 41 | 4.08 | 0.01 | 2.0 | Br10 | N | 80 | 410 | H |
δ Eri | 0.13 | 0.08 | 13 | 5045 | 65 | 3.77 | 0.02 | 0.7 | Br10 | N | 80 | 350 | H, U, U.P |
ϵ Eri | –0.07 | 0.05 | 17 | 5050 | 42 | 4.60 | 0.03 | 2.4 | VF05 | U.P | 80 | 1560 | H, U |
ϵ For | –0.62 | 0.12 | 9 | 5069 | 78 | 3.45 | 0.05 | 4.2 | Schr | H | 115 | 310 | – |
ϵ Vir | 0.12 | 0.03 | 3 | 4983 | 61 | 2.77 | 0.01 | 2.0 | Hekk | N | 80 | 380 | H |
η Boo | 0.25 | 0.04 | 9 | 6105 | 28 | 3.80 | 0.02 | 12.7 | Br10 | N | 80 | 430 | H |
γ Sge | –0.31 | 0.09 | 2 | 3807 | 49 | 1.05 | 0.10 | 6.0 | Hekk | N | 80 | 460 | – |
Gmb 1830 | -1.34 | 0.08 | 17 | 4827 | 55 | 4.60 | 0.03 | 0.5 | VF05 | N | 80 | 410 | – |
HD 107328 | –0.30 | 0.00 | 1 | 4590 | 59 | 2.20 | 0.07 | 1.9 | Mass | N | 80 | 380 | H |
HD 122563 | –2.59 | 0.14 | 7 | 4608 | 60 | 1.61 | 0.07 | 5.0 | Me06 | N | 80 | 300 | H, U, U.P |
HD 140283 | –2.41 | 0.10 | 10 | 5720 | 120 | 3.67 | 0.04 | 5.0 | Me06 | N | 80 | 320 | H, U, U.P |
HD 220009 | –0.67 | 0.00 | 1 | 4266 | 54 | 1.43 | 0.10 | 1.0 | Me99 | N | 80 | 380 | – |
HD 22879 | –0.85 | 0.04 | 16 | 5786 | 89 | 4.23 | 0.03 | 4.4 | Schr | N | 80 | 300 | – |
HD 49933 | –0.39 | 0.07 | 5 | 6635 | 91 | 4.21 | 0.03 | 10.0 | Br09 | H | 115 | 310 | – |
HD 84937 | –2.08 | 0.09 | 13 | 6275 | 97 | 4.11 | 0.06 | 5.2 | Me06 | H | 115 | 480 | N, U, U.P |
ξ Hya | 0.21 | 0.00 | 1 | 5044 | 38 | 2.87 | 0.01 | 2.4 | Br10 | H | 115 | 370 | – |
μ Ara | 0.29 | 0.04 | 12 | 5845 | 66 | 4.27 | 0.02 | 2.3 | Br10 | U | 105 | 420 | |
μ Cas A | –0.89 | 0.04 | 14 | 5308 | 29 | 4.41 | 0.02 | 0.0 | Luck | N | 80 | 280 | U |
μ Leo | 0.39 | 0.10 | 4 | 4433 | 60 | 2.50 | 0.07 | 5.1 | Hekk | N | 80 | 400 | – |
Procyon | –0.02 | 0.04 | 18 | 6545 | 84 | 3.99 | 0.02 | 2.8 | Br10 | U.P | 80 | 760 | N, H, U |
ψ Phe | – | – | 0 | 3472 | 92 | 0.62 | 0.11 | 3.0 | Zama | U | 70 | 220 | – |
Sun | 0.00 | 0.00 | 0 | 5777 | 1 | 4.43 | 2E-4 | 1.6 | VF05 | H | 115 | 350 | H, N, U* * |
τ Cet | –0.53 | 0.05 | 17 | 5331 | 43 | 4.44 | 0.02 | 1.1 | Saar | N | 80 | 360 | H |
Notes. Column description: [Fe/H]LIT corresponds to the mean value of the metallicity obtained by works between 2000 and 2012 as retrieved from PASTEL (Soubiran et al. 2010), where σ[Fe/H] is the standard deviation of the mean and N represents the number of works considered for the mean calculation (see Sect. 2). Effective temperature, surface gravity and their respective uncertainties are determined from fundamental relations as in Paper I, and the rotational velocity v sini is taken from literature with Ref representing the source of this value. The column Source indicates the instrument used to observe the spectrum in the 70 k library (see Sect. 4.2), where N, H, U, and U.P denote NARVAL, HARPS, UVES and UVES-POP spectra, respectively. The column R and S/N represent the resolving power and averaged signal-to-noise ratio of the spectra of the original library (see Sect. 4.2), respectively. For stars repeated in the complete 70 k library (see Sect. 4.2), the extra source are indicated in the column labeled as “extra spectra”.
There are many spectra of the Sun taken from different asteroids for HARPS and NARVAL (see Paper II for details of the library).
Reference. (Saar) Saar & Osten (1997); (Benz) Benz & Mayor (1984); (Br10) Bruntt et al. (2010); (Zama) Zamanov et al. (2008); (Hekk) Hekker & Meléndez (2007); (Me02) De Medeiros et al. (2002); (Re03) Reiners & Schmitt (2003); (VF05) Valenti & Fischer (2005); (Schr) Schröder et al. (2009); (Mass) Massarotti et al. (2008); (Me06) De Medeiros et al. (2006); (Me99) De Medeiros & Mayor (1999); (Br09) Bruntt (2009).
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