Table 2
Seismic solar analogs observed by Kepler and their derived stellar properties.
| # star | KIC | M (M⊙) | R (R⊙) | Age (Gyr) | Teff (K) | log g | Δν (μHz) | Ref. | Sources |
|
|
|||||||||
| 1 | 3241581 | 0.89 ± 0.12 | 1.03 ± 0.05 | 10.5 ± 5.0 | 5770 ± 81 | 4.36 ± 0.02 | 122.9 ± 1.6 | 1 | 1 |
| 2 | 3656476 | 1.09 ± 0.01 | 1.32 ± 0.03 | 7.7 ± 0.2 | 5710 ± 84 | 4.22 ± 0.01 | 93.3 ± 1.3 | 3 | 1, 2, 3 |
| 3 | 4914923 | 1.10 ± 0.01 | 1.37 ± 0.05 | 6.2 ± 0.2 | 5905 ± 84 | 4.21 ± 0.01 | 88.6 ± 0.3 | 3 | 3 |
| 4 | 5084157 | 1.06 ± 0.13 | 1.36 ± 0.08 | 7.8 ± 3.4 | 5803 ± 83 | 4.19 ± 0.02 | 87.3 ± 2.6 | 1 | 1 |
| 5 | 5774694 | 1.06 ± 0.05 | 1.00 ± 0.03 | 1.9 ± 1.8 | 5875 ± 84 | 4.46 ± 0.02 | 140.2 ± 4.0 | 2 | 2 |
| 6 | 6116048 | 1.01 ± 0.03 | 1.22 ± 0.01 | 6.2 ± 0.4 | 5935 ± 84 | 4.27 ± 0.01 | 100.9 ± 1.4 | 4 | 2, 3, 4 |
| 7 | 6593461 | 0.94 ± 0.16 | 1.29 ± 0.07 | 10.7 ± 4.4 | 5817 ± 101 | 4.19 ± 0.02 | 90.8 ± 2.0 | 1 | 1 |
| 8† | 7296438 | 0.91 ± 0.15 | 1.30 ± 0.06 | 12.3 ± 4.3 | 5749 ± 56 | 4.17 ± 0.03 | 88.6 ± 2.1 | 1 | 1 |
| 9 | 7680114 | 1.12 ± 0.07 | 1.43 ± 0.04 | 6.5 ± 1.5 | 5855 ± 84 | 4.18 ± 0.01 | 85.1 ± 1.3 | 2 | 1, 2 |
| 10 | 7700968 | 1.00 ± 0.12 | 1.21 ± 0.06 | 7.5 ± 3.1 | 5982 ± 75 | 4.27 ± 0.02 | 102.6 ± 2.9 | 1 | 1 |
| 11 | 9049593 | 1.13 ± 0.14 | 1.40 ± 0.06 | 6.4 ± 3.4 | 5788 ± 59 | 4.19 ± 0.02 | 86.3 ± 2.1 | 1 | 1 |
| 12 | 9098294 | 1.00 ± 0.03 | 1.15 ± 0.01 | 7.3 ± 0.5 | 5840 ± 84 | 4.30 ± 0.01 | 108.8 ± 1.7 | 4 | 1, 2, 4 |
| 13 | 10130724 | 0.85 ± 0.12 | 1.08 ± 0.05 | 13.8 ± 5.0 | 5648 ± 70 | 4.31 ± 0.02 | 112.9 ± 1.6 | 1 | 1 |
| 14 | 10215584 | 0.99 ± 0.13 | 1.12 ± 0.05 | 6.8 ± 3.5 | 5995 ± 57 | 4.34 ± 0.02 | 114.7 ± 3.1 | 1 | 1 |
| 15 | 10644253 | 1.13 ± 0.05 | 1.11 ± 0.02 | 1.1 ± 0.2 | 6030 ± 84 | 4.40 ± 0.01 | 123.6 ± 2.7 | 4 | 2, 4 |
| 16 | 10971974 | 1.04 ± 0.12 | 1.19 ± 0.06 | 5.8 ± 3.0 | 6030 ± 58 | 4.30 ± 0.02 | 106.2 ± 3.5 | 1 | 1 |
| 17† | 11127479 | 1.14 ± 0.12 | 1.36 ± 0.06 | 5.1 ± 2.2 | 5998 ± 57 | 4.22 ± 0.01 | 90.6 ± 2.5 | 1 | 1 |
| 18 | 11971746 | 1.11 ± 0.14 | 1.35 ± 0.06 | 6.0 ± 2.8 | 5952 ± 75 | 4.22 ± 0.02 | 90.8 ± 2.1 | 1 | 1 |
Notes. The two stars indicated by the symbol (†) a re candidates for hosting a planetary system from the Kepler Objects of Interest (KOI) list (source: MAST at https://archive.stsci.edu/kepler/). From the analysis of spectroscopic Hermes observations, Beck et al. (2015) found for KIC 3241581 the following values: Teff = 5769 ± 4 K, log g = 4.39 ± 0.01, M = 1.03 ± 0.10 M⊙, and R = 1.08 ± 0.10 R⊙, and Salabert et al. (2016) found for KIC 10644253: Teff = 6006 ± 100 K, and log g = 4.3 ± 0.1.
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