Table B.2.
12 γ Dor stars with identified SNFs also have been observed using Kepler’s short cadence.
| KIC | Nquarter | NSNF | NLC | NSC |
|---|---|---|---|---|
| 2168333 | 1 | 8 | 509 | 47 |
| 3967333 | 1 | 6 | 238 | 52 |
| 4480321 | 1 | 3 | 212 | 10 |
| 5219533 | 1 | 1 | 333 | 10 |
| 5476864 | 1 | 1 | 73 | 10 |
| 6614168 | 1 | 1 | 283 | 26 |
| 7748238 | 6 | 2 | 203 | 102 |
| 7770282 | 1 | 2 | 16 | 45 |
| 7977996 | 1 | 19 | 583 | 59 |
| 9533489 | 2 | 8 | 56 | 36 |
| 9651065 | 2 | 17 | 430 | 273 |
| 10647493 | 1 | 1 | 47 | 116 |
Notes. Nquarter represents the number of quarters with short-cadence data; Nsnf denotes the number of SNFs; NLC denotes the number of frequencies detected in long-cadence data with a S/N greater than 8; and NSC cdenotes the number of frequencies detected in short-cadence data with an S/N greater than 8.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.