List of objects with detected rotational splittings, also shown in Fig. 6. For each object, we list the frequency that form the multiplet (column 2), the value of the Ckℓ obtained from the asteroseismological representative model (column 3), and the mean rotation period (column 4).
| TIC . | ν [|$\mu$|Hz] . | Ckℓ . | |$\bar{P}_{\rm rot}$| . |
|---|---|---|---|
| 7675859 | 2830.86, 2808.28, 2775.31 | 0.487 | 5.20 h |
| 21187072 | 933.93, 930.86, 928.63 | 0.495 | 2.24 d |
| 343296348 | 3481.29, 3475.12, 3468.97 | 0.458 | 1.02 d |
| 394015496 | 3233.00, 3227.99, 3223.00 | 0.463 | 1.24 d |
| TIC . | ν [|$\mu$|Hz] . | Ckℓ . | |$\bar{P}_{\rm rot}$| . |
|---|---|---|---|
| 7675859 | 2830.86, 2808.28, 2775.31 | 0.487 | 5.20 h |
| 21187072 | 933.93, 930.86, 928.63 | 0.495 | 2.24 d |
| 343296348 | 3481.29, 3475.12, 3468.97 | 0.458 | 1.02 d |
| 394015496 | 3233.00, 3227.99, 3223.00 | 0.463 | 1.24 d |
List of objects with detected rotational splittings, also shown in Fig. 6. For each object, we list the frequency that form the multiplet (column 2), the value of the Ckℓ obtained from the asteroseismological representative model (column 3), and the mean rotation period (column 4).
| TIC . | ν [|$\mu$|Hz] . | Ckℓ . | |$\bar{P}_{\rm rot}$| . |
|---|---|---|---|
| 7675859 | 2830.86, 2808.28, 2775.31 | 0.487 | 5.20 h |
| 21187072 | 933.93, 930.86, 928.63 | 0.495 | 2.24 d |
| 343296348 | 3481.29, 3475.12, 3468.97 | 0.458 | 1.02 d |
| 394015496 | 3233.00, 3227.99, 3223.00 | 0.463 | 1.24 d |
| TIC . | ν [|$\mu$|Hz] . | Ckℓ . | |$\bar{P}_{\rm rot}$| . |
|---|---|---|---|
| 7675859 | 2830.86, 2808.28, 2775.31 | 0.487 | 5.20 h |
| 21187072 | 933.93, 930.86, 928.63 | 0.495 | 2.24 d |
| 343296348 | 3481.29, 3475.12, 3468.97 | 0.458 | 1.02 d |
| 394015496 | 3233.00, 3227.99, 3223.00 | 0.463 | 1.24 d |
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