Table 1
Characteristic parameters of the red giants named in the paper.
| KIC number | Δν | νmaxa | ΔΠ1b | q | Rseisc | Mseisc | Evolutionary |
| (μHz) | (μHz) | (s) | (R⊙) | (M⊙) | statusd | ||
|
|
|||||||
| 2013502 | 5.72 | 61.2 | 232.20 ± 0.10 | 0.27 ± 0.03 | 10.12 | 1.87 | 2nd clump |
| 3744043 | 9.90 | 110.9 | 75.98 ± 0.10 | 0.16 ± 0.03 | 6.24 | 1.32 | RGB |
| 4044238 | 4.07 | 33.7 | 296.35 ± 0.15 | 0.32 ± 0.05 | clump | ||
| 5000307 | 4.74 | 42.2 | 323.70 ± 0.30 | 0.26 ± 0.06 | 10.36 | 1.38 | clump |
| 6928997 | 10.06 | 120.0 | 77.21 ± 0.02 | 0.14 ± 0.04 | 6.36 | 1.44 | RGB |
| 8378462 | 7.27 | 90.3 | 238.30 ± 0.20 | 0.23 ± 0.05 | 9.39 | 2.42 | 2nd clump |
| 9332840 | 4.39 | 41.4 | 298.9 ± 0.2–306.3 ± 0.2 | 0.20 ± 0.05 | 11.67 | 1.69 | clump |
| 9882316 | 13.68 | 179.3 | 80.58 ± 0.02 | 0.15 ± 0.05 | 5.41 | 1.63 | RGB |
Notes. Asymptotic mixed-mode parameters of the red giant oscillation spectra shown in the paper. The complete table can be downloaded at the CDS.
Mseis and Rseis are the asteroseismic estimates of the stellar mass and radius from scaling relations, using Teff from the Kepler Input Catalog (Brown et al. 2011).
The division between RGB and clump stars is derived from Fig. 3; the limit between the primary and secondary (2nd clump) clump stars is set at 1.8 M⊙.
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