Table 3
Stellar frequencies and amplitudes of δ-Scuti KIC 9700322 measured using our algorithm and using the prewhitening program period04 (Breger et al. 2011).
| f# | fLASR (μ Hz ) | fPERIOD04 (μ Hz ) | aLASR (10-3) | aPERIOD04 (10-3) |
|---|---|---|---|---|
| 1 | 145.473 ± 1.8e–5 | 145.472 | 29.391 ± 0.003 | 29.463 |
| 2 | 113.339 ± 2e–5 | 113.339 | 27.268 ± 0.003 | 27.266 |
| 3 | 258.811 ± 8e–5 | 258.812 | 4.899 ± 0.003 | 4.902 |
| 4 | 290.945 ± 0.00015 | 290.945 | 2.665 ± 0.003 | 2.663 |
| 5 | 32.1338 ± 0.0002 | 32.133 | 2.637 ± 0.003 | 2.633 |
| ... | ... | ... | ... | ... |
| 72 | 727.361 ± 0.014 | 727.362 | 0.015 ± 0.003 | 0.019 |
| 73 | 263.59 ± 0.02 | 263.588 | 0.014 ± 0.003 | 0.015 |
| 74 | 392.96 ± 0.02 | 393.002 | 0.0141 ± 0.003 | 0.015 |
| 75 | 289.09 ± 0.02 | 289.096 | 0.0135 ± 0.003 | 0.016 |
| 76 | 598.96 ± 0.02 | 598.982 | 0.0126 ± 0.003 | 0.014 |
Notes.We find that LASR and prewhitening produce almost identical results with little or no discrepancy between frequency and amplitude values. Breger et al. (2011) list their frequency uncertainty as 0.001 μ Hz and amplitude uncertainty as 0.003 for all modes of oscillation.
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