Table 7.
Observational constraints for the second category of LEGACY targets.
| KIC | Nickname | Teff | [Fe/H] | L | νmax | References |
|---|---|---|---|---|---|---|
| (K) | (dex) | (L⊙) | (μHz) | |||
| 6116048 | Nunny | 6033 ± 100 | −0.23 ± 0.10 | 1.85 ± 0.07 | 2126.9 ± 5.3 | 1 |
| 6225718 | Saxo2 | 6203 ± 100 | −0.17 ± 0.10 | 2.13 ± 0.08 | 2364.2 ± 4.8 | 2 |
| 8006161 | Doris | 5488 ± 100 | 0.34 ± 0.10 | 0.69 ± 0.03 | 3574.7 ± 11.0 | 1 |
| 8379927 | Arthur | 6067 ± 150 | −0.10 ± 0.15 | – | 2795.3 ± 6.0 | 3 |
| 9139151 | Carlsberg | 6043 ± 100 | 0.05 ± 0.10 | 1.60 ± 0.06 | 2690.4 ± 11.8 | 2 |
| 10454113 | Pinocha | 6177 ± 100 | −0.07 ± 0.10 | – | 2357.2 ± 8.7 | 1 |
| 12009504 | Dushera | 6179 ± 100 | −0.08 ± 0.10 | 2.70 ± 0.11 | 1865.6 ± 7.0 | 1 |
| 12258514 | Barney | 5964 ± 60 | 0.00 ± 0.10 | 2.95 ± 0.11 | 1512.7 ± 3.1 | 1 |
Notes. (1) Lund et al. (2017); (2) frequencies and νmax from Lund et al. (2017), Teff and [Fe/H] from Furlan et al. (2018); (3) frequencies from Roxburgh (2017), Teff, [Fe/H], and νmax from Lund et al. (2017). The luminosity L is estimated using the spectroscopic parameters and Eq. (13). For Arthur, the RUWE Gaia indicator flags the parallax measurement as unreliable, and for Pinocha, the Ks-magnitude measurement is unreliable. Therefore, we could not estimate the absolute luminosity of these two targets reliably.
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