Table 4
Frequency content of the KIC 9533489 Kepler data.
| Frequency | Ampl. | Phase | S/N | sig | Combinations | |||
| [d-1] | Δf a | [μHz] | [ppt] | [2π] | ||||
|
|
||||||||
| f1 | 4.007089(4) | –0.04 | 46.37834 | 0.333 | 0.566 | 186.2 | 9967.3 | |
| f2 | 4.443236(4) | 0.10 | 51.42635 | 0.322 | 0.039 | 180.3 | 10 647.4 | |
| f3 | 3.60269(1) | –0.23 | 41.6978 | 0.120 | 0.185 | 67.3 | 1747.5 | |
| f4 | 2.87088(1) | –0.33 | 33.2277 | 0.116 | 0.947 | 64.6 | 1693.5 | |
| f5 | 3.68992(1) | 0.12 | 42.7075 | 0.113 | 0.940 | 63.1 | 1646.5 | |
| f6 | 10.08357(1) | 0.27 | 116.7080 | 0.102 | 0.850 | 59.0 | 1385.9 | |
| f7 | 32.58125(2) | 377.0979 | 0.080 | 0.506 | 46.7 | 850.6 | ||
| f8 | 31.65313(2) | 366.3557 | 0.065 | 0.275 | 38.0 | 580.5 | ||
| f9 | 30.19377(2) | 349.4650 | 0.064 | 0.562 | 37.2 | 563.3 | ||
| f10 | 3.77254(2) | 0.04 | 43.6637 | 0.057 | 0.884 | 31.6 | 446.9 | |
| f11 | 32.35529(2) | 374.4825 | 0.055 | 0.554 | 32.4 | 432.9 | ||
| f12 | 6.36563(2) | 0.18 | 73.6763 | 0.053 | 0.597 | 29.8 | 395.0 | |
| f13 | 1.15926(3) | –0.05 | 13.4173 | 0.052 | 0.243 | 28.7 | 374.6 | |
| f14 | 1.87679(3) | –0.22 | 21.7221 | 0.044 | 0.401 | 24.7 | 280.3 | |
| f15 | 2.50313(3) | 0.38 | 28.9714 | 0.042 | 0.670 | 23.4 | 253.5 | |
| f16 | 1.51617(5) | 1.11 | 17.5483 | 0.041 | 0.103 | 23.0 | 254.1 | |
| f17 | 29.73612(3) | 344.1680 | 0.039 | 0.163 | 22.7 | 217.2 | ||
| f18 | 8.75884(4) | 0.71 | 101.3754 | 0.034 | 0.383 | 19.6 | 173.6 | |
| f19 | 3.38343(5) | –0.99 | 39.1601 | 0.029 | 0.698 | 16.0 | 121.7 | |
| f20 | 7.37521(5) | –0.66 | 85.3612 | 0.028 | 0.557 | 15.8 | 115.7 | f3 + f10 |
| f21 | 35.37792(5) | 409.4667 | 0.025 | 0.664 | 14.8 | 94.6 | ||
| f22 | 37.60866(5) | 435.2854 | 0.024 | 0.258 | 14.3 | 86.0 | ||
| f23 | 11.92258(6) | 0.15 | 137.9929 | 0.022 | 0.674 | 13.0 | 72.6 | |
| f24 | 8.57253(6) | 0.95 | 99.2191 | 0.022 | 0.654 | 12.3 | 70.2 | |
| f25 | 27.04778(6) | 313.0530 | 0.021 | 0.033 | 12.1 | 62.9 | ||
| f26 | 33.05026(7) | 382.5261 | 0.019 | 0.553 | 11.0 | 51.5 | ||
| f27 | 3.89026(7) | –0.58 | 45.0261 | 0.019 | 0.298 | 10.5 | 51.2 | |
| f28 | 0.83999(7) | 2.10 | 9.7221 | 0.019 | 0.780 | 10.2 | 49.5 | f2−f3 |
| f29 | 1.67951(7) | –1.71 | 19.4388 | 0.018 | 0.575 | 9.8 | 46.1 | (2f28) |
| f30 | 8.02468(7) | 0.40 | 92.8782 | 0.017 | 0.135 | 9.7 | 43.6 | |
| f31 | 12.39149(8) | –1.47 | 143.4200 | 0.016 | 0.053 | 9.5 | 39.1 | |
| f32 | 5.22971(9) | –0.04 | 60.5291 | 0.015 | 0.166 | 8.4 | 33.3 | |
| f33 | 5.60943(9) | 1.87 | 64.9240 | 0.014 | 0.787 | 7.9 | 29.4 | |
| f34 | 1.56217(9) | –1.43 | 18.0806 | 0.014 | 0.512 | 7.9 | 28.4 | |
| f35 | 14.5764(1) | –0.37 | 168.708 | 0.012 | 0.650 | 7.2 | 22.6 | |
| f36 | 3.6622(1) | –0.95 | 42.387 | 0.012 | 0.135 | 6.9 | 22.1 | f13 + f15 |
| f37 | 33.6440(1) | 389.398 | 0.012 | 0.977 | 6.9 | 19.9 | ||
| f38 | 2.5311(1) | –0.72 | 29.295 | 0.010 | 0.532 | 5.7 | 15.9 | f5−f13 |
| f39 | 7.9278(1) | –1.43 | 91.757 | 0.010 | 0.868 | 5.8 | 16.2 | f12 + f34 |
| f40 | 6.6502(1) | 2.25 | 76.970 | 0.010 | 0.425 | 5.8 | 15.5 | |
| f41 | 7.7748(1) | –1.34 | 89.986 | 0.010 | 0.261 | 5.6 | 14.7 | |
| f42 | 35.0501(1) | 405.673 | 0.010 | 0.286 | 5.8 | 14.4 | ||
| f43 | 1.1769(2) | 0.69 | 13.622 | 0.009 | 0.357 | 5.1 | 13.1 | |
| f44 | 2.1616(1) | 0.65 | 25.018 | 0.009 | 0.397 | 5.1 | 12.7 | f11−f9 |
| f45 | 4.8035(1) | –0.17 | 55.596 | 0.009 | 0.145 | 5.0 | 11.9 | f12−f34 |
| f46 | 1.2225(2) | –1.07 | 14.150 | 0.009 | 0.514 | 4.8 | 10.9 | f32−f1 |
| f47 | 3.3593(2) | 0.75 | 38.881 | 0.008 | 0.586 | 4.6 | 9.9 | (4f28) |
| f48 | 1.1976(2) | 4.00 | 13.861 | 0.008 | 0.381 | 4.5 | 8.0 | |
| f49 | 8.8862(2) | –2.26 | 102.850 | 0.008 | 0.775 | 4.7 | 9.8 | 2f2 |
| f50 | 34.1421(2) | 395.163 | 0.008 | 0.003 | 4.8 | 9.9 | f7 + f34 | |
| f51 | 1.5106(2) | –5.66 | 17.483 | 0.008 | 0.180 | 4.5 | 8.6 | f6−f24 |
| f52 | 2.5667(2) | 0.99 | 29.707 | 0.008 | 0.992 | 4.4 | 9.2 | f2−f14 |
| f53 | 2.2978(2) | 3.10 | 26.595 | 0.007 | 0.382 | 4.1 | 8.0 | |
| f54 | 31.8377(2) | 368.492 | 0.007 | 0.223 | 4.3 | 8.0 | ||
| f55 | 1.2767(2) | 0.03 | 14.776 | 0.007 | 0.494 | 4.1 | 7.8 | |
Notes. The errors given in parentheses are standard uncertainties derived from the least-squares fitting. We present the frequencies, amplitudes, and phases derived from the SC light curve because the SC data allow the direct detection of peaks above 24.5 d-1. Furthermore, we list the frequency differences of the SC and LC frequencies in the third column. The spectral significances (sig) were calculated using SigSpec (Reegen 2007).
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