Table 4.
EC 23487-2424: results of the fit of the data set with 14 frequencies derived by the ultrashort cadence mode TESS observations (‘This work’).
| This work |
P01 – Bognár et al. (2020) |
||||||
|---|---|---|---|---|---|---|---|
| Frequency | Period | Ampl. | Frequency | Period | Ampl. | Sel. | |
| [μHz] | [s] | [mma] | [μHz] | [s] | [mma] | ||
| 1103.005(39) | 906.615 | 2.65(45) | |||||
| 1104.293(37) | 905.557 | 2.84(45) | f1 | x | |||
 |
1139.799(34) | 877.348 | 3.30(49) | x | |||
| 1144.365(35) | 873.847 | 3.00(45) |
 |
1144.67(35)* | 873.614 | 1.61(30) | x |
| 1175.997(31) | 850.342 | 3.31(45) | f3 | x | |||
| 1208.947(35) | 827.166 | 2.99(45) | f4 | 1206.495(39)* | 828.847 | 2.41(05) | x |
| 1355.178(30) | 737.910 | 3.52(46) | |||||
| 1355.546(26) | 737.710 | 4.06(46) | f5 | x | |||
 |
1367.082(17) | 731.485 | 6.65(49) | ||||
| 1371.708(24) | 729.018 | 4.30(46) | |||||
| 1372.103(22) | 728.808 | 4.67(46) | f6 | 1372.116(35) | 728.802 | 3.15(49) | x |
 |
1376.720(39) | 726.364 | 2.81(49) | ||||
| 1428.764(30) | 699.906 | 3.51(47) | |||||
| 1429.206(20) | 699.689 | 5.32(47) | |||||
| 1430.753(33) | 698.933 | 3.15(46) | f7 | 1430.780(17) | 698.920 | 6.41(49) | x |
| 1431.165(24) | 698.731 | 4.30(47) | |||||
| f8 | 1589.850(37) | 628.990 | 2.96(49) | x | |||
| f9 | 1708.434(27) | 585.331 | 4.05(49) | x | |||
| 1958.384(26) | 510.625 | 4.15(49) |
 |
x | |||
 |
1963.783(23) | 509.221 | 4.88(49) | x | |||
Notes. The errors are formal uncertainties. P01 frequencies: the results of Lorentzian fits are marked with an asterisk. We also present a possible frequency identification in Col. 4. In the case of the supposed rotationally split frequencies, we mark the possible azimuthal order values. We use an ‘x’ to mark the frequencies selected for asteroseismic period fits.
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