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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.

(a)

νmax indicates the central frequency of the oscillation power excess.

(b)

This uncertainty assumes that εg is fixed to 1/2.

(c)

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).

(d)

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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