Table B.1
Rotation rates frot and asymptotic period spacings ΔΠl computed from the observed period spacing patterns, as well as the mode identification and the dominant pulsation frequency for each series.
| KIC | l | m | f dom,inert | f rot | ΔΠl | | s | | |||
| [d-1] | [μHz] | [d-1] | [μHz] | [s] | [d] | ||||
|
|
|||||||||
| 2710594 | 1 | 1 |
|
|
|
|
|
|
|
| R | R |
|
|
|
|
|
|
|
|
| 3448365 | 1 | 1 |
|
|
|
|
|
|
|
| R | R |
|
|
|
|
|
|
|
|
| 4846809 | 1 | 1 |
|
|
|
|
|
|
|
| 1 | 0 |
|
|
|
|
|
|
|
|
| 5114382 | 1 | 1 |
|
|
|
|
|
|
|
| R | R |
|
|
|
|
|
|
|
|
| 5522154 | 1 | 1 |
|
|
|
|
|
|
|
| 5708550 | 1 | 1 |
|
|
|
|
|
|
|
| 5788623 | 1 | 1 |
|
|
|
|
|
|
|
| 6468146 | 1 | 1 |
|
|
|
|
|
|
|
| 6468987 | 1 | 1 |
|
|
|
|
|
|
|
| R | R |
|
|
|
|
|
|
|
|
| 6678174 | 1 | 1 |
|
|
|
|
|
|
|
| 6935014 | 1 | 1 |
|
|
|
|
|
|
|
| 6953103 | 1 | 1 |
|
|
|
|
|
|
|
| 7023122 | 1 | 1 |
|
|
|
|
|
|
|
| 7365537 | 1 | 1 |
|
|
|
|
|
|
|
| S | S |
|
|
|
|
|
|
|
|
| 7380501 | 1 | 1 |
|
|
|
|
|
|
|
| 7434470 | 1 | 1 |
|
|
|
|
|
|
|
| S | S |
|
|
|
|
|
|
|
|
| 7583663 | 1 | 1 |
|
|
|
|
|
|
|
| R | R |
|
|
|
|
|
|
|
|
| 7746984 | 1 | 1 |
|
|
|
|
|
|
|
| S | S |
|
|
|
|
|
|
|
|
| 7939065 | 1 | 1 |
|
|
|
|
|
|
|
| 8364249 | 1 | 1 |
|
|
|
|
|
|
|
| 8375138 | 1 | 1 |
|
|
|
|
|
|
|
| R | R |
|
|
|
|
|
|
|
|
| 8645874 | 1 | 1 |
|
|
|
|
|
|
|
| 8836473 | 1 | 1 |
|
|
|
|
|
|
|
| S | S |
|
|
|
|
|
|
|
|
| 9210943 | 1 | 1 |
|
|
|
|
|
|
|
| R | R |
|
|
|
|
|
|
|
|
| 9480469 | 1 | 1 |
|
|
|
|
|
|
|
| R | R |
|
|
|
|
|
|
|
|
| 9595743 | 1 | 1 |
|
|
|
|
|
|
|
| 1 | 0 |
|
|
|
|
|
|
|
|
| 9751996 | 1 | 1 |
|
|
|
|
|
|
|
| 1 | 0 |
|
|
|
|
|
|
|
|
| 1 | − 1 |
|
|
|
|
|
|
|
|
| 10256787 | 1 | 1 |
|
|
|
|
|
|
|
| 10467146 | 1 | 1 |
|
|
|
|
|
|
|
| 11080103 | 1 | 1 |
|
|
|
|
|
|
|
| 11099031 | 1 | 1 |
|
|
|
|
|
|
|
| S | S |
|
|
|
|
|
|
|
|
| 11294808 | 1 | 1 |
|
|
|
|
|
|
|
| 2 | 2 |
|
|
|
|
|
|
|
|
| 11456474 | 1 | 1 |
|
|
|
|
|
|
|
| 11721304 | 1 | 1 |
|
|
|
|
|
|
|
| 11754232 | 1 | 1 |
|
|
|
|
|
|
|
| 11826272 | 1 | 1 |
|
|
|
|
|
|
|
| 11907454 | 1 | 1 |
|
|
|
|
|
|
|
| R | R |
|
|
|
|
|
|
|
|
| 11917550 | 1 | 1 |
|
|
|
|
|
|
|
| 11920505 | 1 | 1 |
|
|
|
|
|
|
|
| 12066947 | 1 | 1 |
|
|
|
|
|
|
|
| R | R |
|
|
|
|
|
|
|
|
Notes. For the latter we also computed the spin parameter s, listed in the final column. The pulsation mode patterns marked with “R” are retrograde modes, which are most likely Rossby modes. The pulsation modes marked with “S” are single high-amplitude peaks that were present in the frequency spectra, but clearly separate from the detected period spacing patterns. Neither the retrograde pulsation modes nor the single peaks were used in the computations. The corresponding rotation rates and asymptotic period spacings were obtained from the prograde series observed for the same star.
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