Table 2.
All detected frequencies along with the corresponding g-modes characterized by angular degree ℓ, radial order ng, and azimuthal order m.
| Frequency | Amplitude | Phase | S/N | l | ng | m | |
|---|---|---|---|---|---|---|---|
| (c/d) | (mmag) | ||||||
| HD 36999 (3.6 M⊙, 25 Myr) | |||||||
| f1 | 1.50460(2) | 10.6(9) | 0.41(1) | 10.6 | 1 | 9 | +1 |
| f2 | 1.43227(2) | 12.6(8) | 0.66(1) | 12.6 | 1 | 9 | −1 |
| f3 | 1.82621(3) | 5.9(9) | 0.84(3) | 5.9 | 1 | 7 | 0 |
| f4 | 7.44114(3) | 4.6(9) | 0.98(3) | 4.3 | 1 | 1 | 0 |
| f5 | 2.61151(3) | 4.9(9) | 0.17(3) | 4.8 | 1 | 5 | 0 |
| HD 48497 (4.2 M⊙, 25 Myr) | |||||||
| f1 | 0.938(2) | 12(4) | 0.8(1) | 7.0 | |||
| f2 | 1.043324(8) | 12(2) | 0.68(2) | 6.6 | 1 | 11 | |
| f3 | 0.89578(6) | 9(2) | 0.01(6) | 5.0 | 1 | 13 | |
| f4 | 1.041(1) | 8(3) | 0.2(1) | 4.5 | 2 | 20 | |
| f5 | 1.265(1) | 8(2) | 0.87(5) | 4.4 | 1 | 9 | |
| HD 61076 (3.2 M⊙, 2 Myr) | |||||||
| f1 | 1.0919(3) | 13(3) | 0.4(2) | 4.2 | 1 | 14 | |
| f2 | 2.73251(1) | 10(1) | 0.35(2) | 4.0 | 1 | 5 | |
| HD 61712 (3.6 M⊙) | |||||||
| f1 | 1.281592(3) | 18.7(7) | 0.422(7) | 25.4 | 1 | 10 | |
| f2 | 1.513(2) | 4(1) | 0.5(2) | 4.7 | 2 | 15 | |
| HD 66181 (75 Myr) | |||||||
| f1 | 0.88522(2) | 14(1) | 0.54(1) | 11.5 | 1 | 12 | +1 |
| f2 | 0.794(8) | 9(4) | 0.4(2) | 7.7 | 1 | 12 | −1 |
| f3 | 0.89936(3) | 8(1) | 0.91(3) | 6.6 | 1 | 11 | 0 |
| f4 | 0.70470(4) | 7(1) | 0.52(3) | 5.7 | 2 | 26 | 0 |
| f5 | 0.84193(3) | 6(1) | 0.54(3) | 4.5 | 1 | 12 | 0 |
| HD 86424 (3.5 M⊙, 50 Myr) | |||||||
| f1 | 1.084518(3) | 12.7(3) | 0.544(3) | 13.2 | 1 | 12 | |
| f2 | 0.10747(1) (a) | 4.4(2) | 0.873(9) | 4.5 | |||
| f3 | 0.95053(4) | 4.9(3) | 0.50(1) | 5.1 | 1 | 14 | |
| HD 97895 (4.8 M⊙, 50 Myr) | |||||||
| f1 | 0.922626(7) | 16.1(3) | 0.667(3) | 7.4 | 1 | 12 | 0 |
| f2 | 0.861588(8) | 15.5(3) | 0.471(3) | 7.6 | 1 | 12 | −1 |
| f3 | 0.98459(1) | 10.1(3) | 0.275(5) | 4.2 | 1 | 12 | +1 |
| f4 | 1.82168(1) | 9.3(3) | 0.611(5) | 4.3 | 1 | 6 | 0 |
| HD 115067 | |||||||
| f1 | 0.62165(2) | 10(1) | 0.15(2) | 7.4 | 1 | >18 | |
| f2 | 0.18665(2) (a) | 7(1) | 0.27(2) | 4.9 | |||
| HD 163285 (3.8 M⊙, 40 Myr) | |||||||
| f1 | 0.82863(1) | 17.0(8) | 0.319(8) | 7.1 | 1 | 15 | |
| f2 | 1.07449(1) | 13.3(8) | 0.22(1) | 5.6 | 1 | 11 | |
| f3 | 1.20341(1) | 11.6(8) | 0.94(1) | 4.9 | 2 | 18 | |
| HD 168121 | |||||||
| f1 | 0.75915(2) | 11(1) | 0.30(2) | 4.9 | |||
| f2 | 0.79316(2) | 10(1) | 0.99(2) | 4.4 | |||
| f3 | 0.77929(2) | 9(1) | 0.06(2) | 4.1 | |||
Notes. Modes were extracted from the best-fit mode combination and stellar model using a grid of models described in Sect. 4. Masses and ages of the stellar models producing the best frequency cross-matches are given in parentheses behind the object identifiers. Age estimation was carried out in cases where models within 0.5 dex of the best-fit model boasted approximately the same age.
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