Table 5.
This work: results of the fit of the EC 23487−2424 data set with ten frequencies.
| This work |
Stobie et al. (1993) | Thompson et al. (2005) | |||
|---|---|---|---|---|---|
| Frequency | Period | Ampl. | Period | Period | |
| [μHz] | [s] | [mma] | [s] | [s] | |
| 993.0 | |||||
| 989.3 | |||||
 |
1139.799(34) | 877.348 | 3.30(49) | 878.8 | |
 |
1144.67(35)* | 873.614 | 1.61(30) | ||
| 868.2 | |||||
| f2 | 1206.495(39)* | 828.847 | 2.41(05) | ||
| 804.5 | |||||
 |
1367.082(17) | 731.485 | 6.65(49) | ||
 |
1372.116(35) | 728.802 | 3.15(49) | ||
 |
1376.720(39) | 726.364 | 2.81(49) | ||
| f4 | 1430.780(17) | 698.920 | 6.41(49) | ||
| f5 | 1589.850(37) | 628.990 | 2.96(49) | ||
| f6 | 1708.434(27) | 585.331 | 4.05(49) | ||
| f7 | 1963.783(23) | 509.221 | 4.88(49) | 508.1 | |
Notes. The errors are formal uncertainties. The results of Lorentzian fits are marked with star symbols (*). In the case of the supposed rotationally split frequencies, we mark the possible azimuthal order values. For completeness, we also list the periods detected by Stobie et al. (1993) and Thompson et al. (2005).
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