Table 11
Mean Teff and log g values from a compilation of spectroscopic, photometric, and parallax-based determinations published between 2000 and 2012.
| Name | Teff | σ | N | Teff | σ | N | log g | σ | N | log g | σ | N |
| [K] | [K] | [cm s-2] | [cm s-2] | |||||||||
| spectroscopic | photometric | spectroscopic | parallax | |||||||||
|
|
||||||||||||
| α Cet | 3834 | 220 | 7 | 3724 | 87 | 2 | 1.29 | 0.43 | 7 | 0.73 | 0.30 | 1 |
| γ Sge | 4064 | 106 | 2 | 3877 | 41 | 1 | 1.52 | 0.32 | 2 | |||
| α Tau | 3987 | 246 | 14 | 3887 | 86 | 2 | 1.42 | 0.31 | 14 | 1.20 | 0.30 | 1 |
| 61 Cyg B | 4400 | 100 | 1 | 4.20 | 0.10 | 1 | ||||||
| HD 220009 | 4402 | 111 | 2 | 4484 | 100 | 1 | 1.95 | 0.34 | 2 | 2.03 | 0.10 | 1 |
| Arcturus | 4326 | 68 | 6 | 4274 | 83 | 5 | 1.70 | 0.20 | 6 | 1.82 | 0.15 | 5 |
| 61 Cyg A | 4655 | 138 | 3 | 4300 | 170 | 2 | 4.49 | 0.17 | 3 | 4.50 | 0.20 | 1 |
| μ Leo | 4590 | 65 | 5 | 4425 | 100 | 1 | 2.65 | 0.22 | 5 | 2.24 | 0.10 | 1 |
| HD 107328 | 4514 | 100 | 1 | 4436 | 125 | 2 | 1.94 | 0.10 | 1 | 2.09 | 0.27 | 2 |
| HD 122563 | 4509 | 75 | 5 | 4795 | 107 | 1 | 1.23 | 0.30 | 4 | 1.44 | 0.24 | 2 |
| Gmb 1830 | 5087 | 100 | 11 | 5133 | 36 | 4 | 4.75 | 0.21 | 9 | 4.69 | 0.05 | 6 |
| β Gem | 4952 | 33 | 4 | 4795 | 87 | 4 | 3.10 | 0.04 | 4 | 2.76 | 0.06 | 3 |
| δ Eri | 5085 | 51 | 9 | 5004 | 20 | 3 | 3.89 | 0.12 | 10 | 3.92 | 0.24 | 3 |
| ϵ Vir | 5115 | 29 | 3 | 5055 | 24 | 3 | 3.05 | 0.11 | 3 | 2.78 | 0.17 | 2 |
| ξ Hya | 5045 | 80 | 1 | 2.81 | 0.08 | 1 | ||||||
| ϵ Eri | 5114 | 68 | 11 | 5063 | 80 | 6 | 4.51 | 0.14 | 12 | 4.61 | 0.02 | 4 |
| ϵ For | 5093 | 14 | 4 | 5135 | 155 | 4 | 4.07 | 0.30 | 5 | 3.61 | 0.10 | 5 |
| α Cen B | 5194 | 33 | 5 | 5131 | 110 | 4 | 4.49 | 0.07 | 5 | 4.58 | 0.06 | 2 |
| μ Cas | 5341 | 92 | 7 | 5338 | 82 | 4 | 4.51 | 0.20 | 8 | 4.62 | 0.09 | 4 |
| τ Cet | 5326 | 45 | 12 | 5395 | 92 | 5 | 4.56 | 0.18 | 14 | 4.62 | 0.07 | 2 |
| HD 140283 | 5692 | 102 | 7 | 5774 | 77 | 7 | 3.54 | 0.15 | 3 | 3.69 | 0.03 | 8 |
| α Cen A | 5816 | 39 | 6 | 5681 | 117 | 6 | 4.30 | 0.13 | 7 | 4.32 | 0.10 | 2 |
| 18 Sco | 5789 | 30 | 9 | 5759 | 72 | 5 | 4.39 | 0.07 | 10 | 4.45 | 0.05 | 4 |
| HD 22879 | 5840 | 73 | 9 | 5844 | 87 | 10 | 4.37 | 0.15 | 8 | 4.33 | 0.10 | 9 |
| β Hyi | 5875 | 87 | 3 | 5815 | 95 | 3 | 4.07 | 0.21 | 4 | 3.98 | 0.03 | 3 |
| μ Ara | 5783 | 46 | 9 | 5703 | 93 | 3 | 4.29 | 0.13 | 9 | 4.26 | 0.12 | 2 |
| β Vir | 6138 | 54 | 6 | 6154 | 89 | 4 | 4.13 | 0.14 | 7 | 4.14 | 0.04 | 3 |
| η Boo | 6085 | 106 | 8 | 6041 | 140 | 2 | 3.94 | 0.18 | 8 | 3.77 | 0.10 | 2 |
| HD 84937 | 6340 | 41 | 7 | 6352 | 63 | 6 | 4.02 | 0.09 | 6 | 4.05 | 0.05 | 6 |
| Procyon | 6601 | 148 | 9 | 6610 | 82 | 6 | 4.16 | 0.30 | 9 | 4.01 | 0.05 | 4 |
| HD 49933 | 6661 | 110 | 5 | 6741 | 106 | 2 | 4.23 | 0.10 | 5 | 4.21 | 0.50 | 1 |
Notes. The stars are ordered by increasing fundamental temperature. Columns headed σ give standard deviations if number of determinations N ≥ 3, or combined linear uncertainties (N = 2) or individual uncertainties (N = 1) quoted in the publications. Teff values from González Hernández & Bonifacio (2009) with uncertainties larger than 200 K due to large uncertainties in 2MASS magnitudes were not included.References for spectroscopic Teff and log g: Smith & Ruck (2000), Mashonkina & Gehren (2000); Fulbright (2000); Westin et al. (2000); Feltzing & Gonzalez (2001); Mishenina & Kovtyukh (2001); Santos et al. (2001); Stephens & Boesgaard (2002); Santos et al. (2003); Laws et al. (2003); Heiter & Luck (2003); Mishenina et al. (2003); Ryan & Smith (2003); Santos et al. (2004); Bruntt et al. (2004); Fuhrmann (2004); Santos et al. (2005); Luck & Heiter (2005); Valenti & Fischer (2005); Takeda et al. (2005); Gillon & Magain (2006); da Silva et al. (2006); Takeda et al. (2007); Hekker & Meléndez (2007); Mashonkina et al. (2008); Sousa et al. (2008); Porto de Mello et al. (2008); Fuhrmann (2008); Bruntt (2009); Gonzalez et al. (2010); Bruntt et al. (2010); da Silva et al. (2011); Sousa et al. (2011); Bruntt et al. (2011); Maldonado et al. (2012); da Silva et al. (2012); Britavskiy et al. (2012); Thygesen et al. (2012); Lebzelter et al. (2012); Pavlenko et al. (2012).References for photometric Teff and parallax-based log g: Nissen et al. (2000); Gratton et al. (2000); Zhao & Gehren (2000); Nissen et al. (2002); Zhao et al. (2002); Allende Prieto et al. (2004); Galeev et al. (2004); Jonsell et al. (2005); Zhang & Zhao (2005); Zhang & Zhao (2006); Kotoneva et al. (2006); Bean et al. (2006); Reddy et al. (2006); Ramírez et al. (2007); Meléndez et al. (2008); Ramírez et al. (2009); Nissen & Schuster (2010); Casagrande et al. (2011).References for spectroscopic Teff and parallax-based log g: Gratton et al. (2003); Korn et al. (2003); Bensby et al. (2003); Gehren et al. (2006); Roederer (2012); Roederer et al. (2012).References for photometric Teff and spectroscopic log g: Bond et al. (2006); Ishigaki et al. (2012).References for photometric Teff only: Ramírez & Meléndez (2005); Masana et al. (2006); González Hernández & Bonifacio (2009); Casagrande et al. (2010); Gebran et al. (2010).References for spectroscopic log g only: Mishenina et al. (2004); Thorén et al. (2004); Kovtyukh et al. (2004).References for parallax-based log g only: Mishenina et al. (2008); Bergemann & Gehren (2008); Ramírez & Allende Prieto (2011).References containing values in three or four categories: Affer et al. (2005); Smiljanic et al. (2007); Luck & Heiter (2007).
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