Table 4
List of stars fulfilling the selection criterion λ1 for showing temporal variability of their p-mode frequency shifts.
| KIC | |Max (δν)|L |  |
p(λ1) | ⟨Sph⟩ | Prot | Category |
|---|---|---|---|---|---|---|
| (μHz) | (μHz) | (%) | (ppm) | (days) | ||
| 5184732* | 0.192 | 0.077 | 84.0 | 222.0 | 19.79 ± 2.43 | simple |
| 6116048† | 0.178 | 0.093 | 75.2 | 87.4 | 17.26 ± 1.96 | simple |
| 7206837 | 0.354 | 0.280 | 43.0 | 246.6 | 4.04 ± 0.28 | simple |
| 7747078 | 0.152 | 0.077 | 84.0 | 176.0 | 17.71 ± 1.78 | mixed-modes |
| 7771282 | 0.431 | 0.396 | 29.7 | 117.6 | 11.88 ± 0.91 | F-like |
| 8006161* | 0.638 | 0.131 | 100.0 | 763.5 | 29.79 ± 3.09 | simple |
| 8150065 | 0.462 | 0.400 | 31.6 | – | – | simple |
| 8379927*,♭ | 0.229 | 0.138 | 51.6 | – | – | simple |
| 8394589 | 0.238 | 0.196 | 32.0 | – | – | simple |
| 8424992 | 0.749 | 0.449 | 36.2 | – | – | simple |
| 9139163‡ | 0.383 | 0.194 | 78.9 | – | – | simple |
| 9206432 | 0.324 | 0.297 | 32.6 | 96.7 | 8.80 ± 1.06 | F-like |
| 9414417 | 0.206 | 0.172 | 37.6 | 146.5 | 22.77 ± 2.37 | F-like |
| 10355856 | 0.469 | 0.227 | 74.0 | 321.5 | 4.47 ± 0.31 | F-like |
| 10454113* | 0.287 | 0.173 | 70.8 | 327.3 | 14.61 ± 1.09 | simple |
| 10730618 | 0.507 | 0.421 | 47.4 | – | – | F-like |
| 10909629 | 0.254 | 0.250 | 31.0 | 55.1 | 12.37 ± 1.22 | F-like |
| 11081729 | 0.601 | 0.521 | 32.3 | 272.2 | 2.74 ± 0.31 | F-like |
| 12009504 | 0.208 | 0.188 | 37.4 | 155.3 | 9.39 ± 0.68 | simple |
| 12069127 | 0.369 | 0.262 | 43.0 | 86.6 | 4.47 ± 0.31 | F-like |
Notes. The
column |Max(δν)|L
corresponds to the maximum linear frequency
shift measured for the stars. The column
gives the mean errors of the extracted frequency shifts. The column
p(λ1 )
gives the percentage for a given star to be
detected according to the simulations. The column
⟨Sph ⟩
corresponds to the mean value of the
Sph (t) proxy
calculated over the duration of the observations. The surface rotation
periods, Prot,
were measured by García et al. (2014a). When no measurements
of Prot
are available, the corresponding values of
Prot and
⟨Sph ⟩ are left
blank. The (*)
indicates the stars which also fulfilled the selection criterion
λ2
. The star KIC 9139163 flagged by the
(‡) has
frequency shifts with a temporal periodicity close to the Kepler
orbital period. The star KIC 6116048 marked with the
(†) is a seismic
solar analog (Salabert et al. 2016). The star KIC 8379927 marked
with the (♭)
is part of a spectroscopic binary system (Pourbaix et
al. 2004).
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