Table 2 Mode frequencies and frequency shifts.

Values of snlm, as defined by Eq. 1, are given for the dipole and quadrupole multiplets in the p-mode range of KIC 11145123. The frequency shifts expected from rotational oblateness, Embedded Image, are computed using Eq. 4. Mode identification is according to the best-fit stellar model, with R = 2.24 R and M = 1.46 M (12). Mode amplitudes are measured to a precision of 0.01 mmag.

nlmνnlm ± σnlm (day−1)Amplitude (mmag)snlm (10−5 day–1)ΔnlEmbedded Image (10−5 day−1)Index
−12−216.7258824 ± 0.0000017 2.33
−116.7339455 ± 0.00001860.21
016.7420104 ± 0.00000750.53
116.7500755 ± 0.00001100.360.1 ± 1.30.40−1.01
216.7580083 ± 0.00005040.08−6.4 ± 2.60.40−3.92
21−118.3558305 ± 0.00000291.36
018.3660001 ± 0.00001350.29
118.3761210 ± 0.00000341.13−2.3 ± 1.40.68−7.73
02−218.9869603 ± 0.00000780.50
−118.9967001 ± 0.00000600.65
019.0064482 ± 0.00000560.69
119.0161736 ± 0.00001010.39−1.1 ± 0.80.39−1.14
219.0259102 ± 0.00000860.45−1.4 ± 0.80.39−4.35
31−121.9933315 ± 0.00000640.61
022.0018915 ± 0.00002860.14
122.0104220 ± 0.00000640.61−1.5 ± 2.90.68−9.26
22−223.5455350 ± 0.00003030.13
−123.5553428 ± 0.00005820.07
023.5651835 ± 0.00004800.08
123.5749885 ± 0.00006070.06−1.7 ± 6.40.20−0.67
223.5847898 ± 0.00001630.24−2.2 ± 5.10.20−2.28