Table 3
Fundamental parameters of the solar analogues from the spectroscopic analysis of Hermes data.
| KIC | T eff | log g | v min | vsini | [Fe/H] | A(Li) | S / N |
| [K] | [dex] | [km s-1] | [km s-1] | [dex] | [dex] | (Li) | |
|
|
|||||||
| 3241581 | 5685±59 | 4.3±0.1 | 1.0±0.2 | 4.0±0.6 | 0.22±0.04 | ≤0.31 | 180 |
| 3656476 | 5674±50 | 4.2±0.1 | 1.1±0.1 | 4.1±0.7 | 0.25±0.04 | ≤0.51 | 120 |
| 4914923 | 5869±74 | 4.2±0.1 | 1.2±0.1 | 5.0±0.6 | 0.12±0.04 | 2.02±0.02 | 175 |
| 5084157 | 5907±60 | 4.2±0.1 | 1.1±0.1 | 4.8±0.7 | 0.24±0.04 | 2.31±0.01 | 85 |
| 5774694 | 5962±59 | 4.6±0.1 | 1.0±0.2 | 5.5±0.7 | 0.10±0.03 | 2.60±0.01 | 190 |
| 6116048 | 6129±97 | 4.3±0.2 | 1.3±0.2 | 5.8±0.6 | −0.18±0.05 | 2.61±0.01 | 150 |
| 6593461 | 5803±126 | 4.4±0.2 | 1.3±0.3 | 4.8±0.8 | 0.25±0.09 | 1.85±0.02 | 70 |
| 7296438 | 5854±64 | 4.3±0.1 | 1.2±0.2 | 4.5±0.8 | 0.24±0.05 | 1.89±0.03 | 80 |
| 7680114 | 5978±107 | 4.3±0.2 | 1.2±0.3 | 4.4±0.7 | 0.15±0.07 | 1.57±0.02 | 135 |
| 7700968 | 5992±144 | 4.4±0.3 | 1.4±0.4 | 5.3±0.7 | −0.18±0.08 | 2.19±0.02 | 100 |
| 9049593 | 6009±151 | 4.3±0.3 | 1.5±0.3 | 7.2±0.6 | 0.20±0.08 | 2.82±0.02 | 95 |
| 9098294 | 5913±67 | 4.4±0.1 | 1.0±0.2 | 4.7±0.7 | −0.14±0.04 | ≤0.86 | 140 |
| 10130724 | 5649±95 | 4.3±0.2 | 0.9±0.3 | 4.4±0.9 | 0.27±0.09 | ≤1.10 | 65 |
| 10215584 | 5888±67 | 4.3±0.1 | 1.1±0.2 | 5.1±0.6 | 0.05±0.04 | 2.25±0.05 | 105 |
| 10644253 | 6117±64 | 4.4±0.2 | 0.9±0.2 | 4.3±0.6 | 0.11±0.04 | 2.99±0.02 | 215 |
| 10971974 | 5895±114 | 4.4±0.2 | 1.2±0.3 | 4.8±0.8 | 0.02±0.07 | ≤1.62 | 55 |
| 11127479 | 5884±116 | 4.4±0.3 | 1.5±0.3 | 6.1±0.7 | 0.11±0.08 | 2.44±0.02 | 50 |
| 11971746 | 5953±63 | 4.3±0.1 | 1.2±0.2 | 4.5±0.8 | 0.18±0.04 | 2.19±0.02 | 105 |
Notes. The star identifier in the Kepler input catalogue, the effective temperature Teff, the surface acceleration log g, the micro turbulence vmin, the projected surface rotational velocity vsini, the stellar metallicity, and the abundance of lithium are given with their respective uncertainties. Upper limits of the measured A(Li) are indicated for stars with low lithium abundance as a consequence of insufficient S/N in the spectra. The last column reports the S/N around the lithium line.
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