Table 2
Low-luminosity red giants with νmax higher than 283 μHz from long cadence data.
| Star | f max | (νmax) | Δν | R | M | log g | L | T eff | P orbit | A | | ΔRV | |
| KIC | [μHz] | [μHz] | [μHz] | [R⊙] | [M⊙] | [dex] | [L⊙] | [K] | [d] | [ppt] | [km s-1] |
|
|
|||||||||||
| 7799540 | 220 ± 5 | (347.2) | 24.0 | 3.64 | 1.52 | 3.50 | 17.5 | 5177 | 71.8 | +0.5 | [31.8] |
| 2697935⋆ | 161 ± 3 | (405.6) | ~28 | 3.26 | 1.45 | 3.574 | 15.7 | 4883 | 21.5 | ±1.3 | 52.1 |
| 8912308 | 217 ± 9 | (350.2) | 22.7 | 4.20 | 2.02 | 3.50 | 23.5 | 4872 | 20.2 | +1.2 | 61.4 |
Notes. The definition of columns KIC, Δν, M, R, log g, L, Porbit, A and Δ | RV | is the same as in Table 1. fmax and (νmax) indicate the frequency of the maximum oscillation power, reflected at the Nyquist frequency and reconstructed power excess, respectively. Teff was adopted from the KIC parameters. The uncertainties of M, R, log g and L are better than 2, 5, 1, and 15 per cent, respectively.
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