Table 6.
BPM 30551: Significant frequencies found in the sector 29 observations (‘This work’).
| This work |
P01 – Bognár et al. (2020) |
||||||
|---|---|---|---|---|---|---|---|
| Frequency [μHz] | Period [s] | Amplitude [mma] | Frequency [μHz] | Period [s] | Amplitude [mma] | Sel. | |
| f1 | 1144.760(150)* | 873.546 | 1.39(03) | x | |||
| 1204.487(021)* | 830.229 | 3.14(02) | |||||
| 1208.880(33) | 827.212 | 3.37(48) | |||||
| 1209.997(27) | 826.448 | 4.17(48) | f2 | x | |||
| f3 | 1264.164(093)* | 789.163 | 1.83(02) | x | |||
| 1413.070(30) | 707.679 | 3.70(49) | f4 | x | |||
| 1487.056(32) | 672.470 | 3.48(49) | f5 | x | |||
| 1490.973(40) | 670.703 | 2.76(49) | |||||
Notes. In the case of the P01 frequencies, they are results of Lorentzian fits to the frequency groups observed in the actual BPM 30551 data set. The central frequencies are marked with asterisks. We use an ‘x’ to mark the frequencies selected for asteroseismic period fits.
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