Table 2

Inferred rotation coefficients and uncertainties for ℓ = 1, | m | = 1 mode splittings with a rotation axis inclination of 90° for independent fits to each star (Cols. 4 and 5); for an ensemble fit for stars with similar synthetic rotation profiles (Cols. 6 and 7); for an ensemble fit for stars with rotation profiles where the rotation rate below the BCZ varied randomly up to 50% from 1035 nHz (Cols. 8 and 9).

			Independent inversions		Ensemble inversions
							Ωc(1 ± 0.5)
T eff	r BCZ	⟨ n ⟩	Ω∗ ± σ(Ω∗)	ΔΩ ± σ(ΔΩ)		ΔΩ ± σ(ΔΩ)		ΔΩ ± σ(ΔΩ)
[K]	[R]		[nHz]	[nHz]	[nHz]	[nHz]	[nHz]	[nHz]
4538	0.65	27	693 ± 552	828 ± 1073	883 ± 173	–111 ± 266	449 ± 173	–111 ± 266
4676	0.64	24	1810 ± 607	–838 ± 720	874 ± 178	–111 ± 266	441 ± 178	–111 ± 266
4860	0.61	22	1632 ± 676	–641 ± 797	866 ± 184	–111 ± 266	324 ± 184	–111 ± 266
5599	0.73	22	1828 ± 587	–1360 ± 1146	876 ± 164	–111 ± 266	1146 ± 164	–111 ± 266
5627	0.67	20	952 ± 699	254 ± 1336	890 ± 166	–111 ± 266	726 ± 166	–111 ± 266
5632	0.71	23	1422 ± 708	–625 ± 1378	865 ± 174	–111 ± 266	904 ± 174	–111 ± 266
5701	0.70	22	–467 ± 723	3056 ± 1394	925 ± 126	–111 ± 266	795 ± 126	–111 ± 266
5744	0.72	20	–230 ± 627	2640 ± 1215	923 ± 137	–111 ± 266	1421 ± 137	–111 ± 266
5892	0.71	18	1823 ± 620	–1358 ± 1195	880 ± 156	–111 ± 266	718 ± 156	–111 ± 266
5983	0.75	19	1649 ± 723	–1078 ± 1405	891 ± 158	–111 ± 266	961 ± 158	–111 ± 266
6252	0.81	19	1382 ± 592	–464 ± 1181	890 ± 162	–111 ± 266	791 ± 162	–111 ± 266
6408	0.84	21	1019 ± 583	271 ± 1170	890 ± 167	–111 ± 266	1733 ± 167	–111 ± 266
6661	0.91	17	942 ± 422	743 ± 1392	949 ± 109	–111 ± 266	493 ± 109	–111 ± 266
6663	0.88	19	380 ± 472	2591 ± 1518	931 ± 102	–111 ± 266	1120 ± 102	–111 ± 266
6680	0.89	18	1121 ± 431	112 ± 1407	942 ± 97	–111 ± 266	1123 ± 97	–111 ± 266