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Table 4
Rotation rate and inclination limits of the HADS candidates in our star sample.
| KIC | A0 (ppm) | νmax (μHz) |  (K) |
Teff (K)a |  (%) |
i (°) |
|---|---|---|---|---|---|---|
| 2857323 | 91200 ± 500 | 180 ± 30 | 7520 ± 100 | 7960 | ≳81 | ≲31 |
| 5950759 | 122700 ± 600 | 210 ± 30 | 7600 ± 100 | 8040 | ≳82 | ≲31 |
| 9408694 | 158400 ± 800 | 90 ± 20 | 7260 ± 70 | 6810 | ≳86 | ≳76 |
Notes. (a) Measured temperaturewith an estimated error of 250 K (Brown et al. 2011; Huber et al. 2014).
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