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Table 2

KIC 10001893: frequency combinations of pulsating modes (Col. 2) derived from various types of data (Col. 1), where data types are: LC (PSF long-cadence light curve ratio of sdBV and the bright neighbor; see Sect. 4 for explanations), SC (aperture sdBV light curve) and UZ (frequencies from Uzundag et al. 2017).

Data nfi – mfj fi, fj ampl. Combination Combination to kl
(μHz) (ppm) (μHz) distance (μHz)
LC 238.9865 (f62) − 224.7199 (f59) 71, 38 14.2666 0.0056(k3)
3 ⋅ 158.0832 (f35) − 3 ⋅ 140.5211 (f29) 155, 138 52.6862 0.0039 (k1)
SC 238.9855 (f62) − 224.7196 (f59) 73, 54 14.2659 0.0049 (k3)
2 ⋅ 114.6710 (f18) − 176.6694 (f44) 34, 34 52.6727 0.0096 (k1)
2 ⋅ 132.4709 (f27) − 3 ⋅ 76.4573 (f) 34, 30 35.5700 0.0096 (k2)
3 ⋅ 181.9716 (f47) − 2 ⋅ 255.1673 (f65) 45, 202 35.5803 0.0007 (k2)
3 ⋅ 158.0832 (f35) − 3 ⋅ 140.5215 (f29) 173, 185 52.6851 0.0029 (k1)
UZ 210.6816 (f55) − 196.4174 (f51)(a) 793, 36 14.2642 0.0033 (k3)
238.9829 (f62) − 224.7191 (f59) 91, 54 14.2638 0.0028 (k3)
3 ⋅ 326.7867 (f75) − 966.0903 (f93) 53, 35 14.2698 0.0088 (k3)
3 ⋅ 201.1749 (f53) − 3 ⋅ 196.4174 (f51)(a) 34, 36 14.2726 0.0116 (k3)
3 ⋅ 158.0828 (f35) − 3 ⋅ 140.5205 (f29) 204, 223 52.6868 0.0045 (k1)

Notes. (a) Frequency close to one of the known Kepler artifacts. Column 2 in round brackets: IDs of the closest match from the Uzundag et al. (2017) frequency list. Column 3: frequency amplitudes from Col. 2. Column 4: combination frequency values. Column 5: distances of k1, k2, and k3 from the frequencies shown in Col. 4. Only pulsating modes with amplitudes greater than 30 ppm are shown.

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