Table 1
Key stellar parameters.
| KIC | HIP | HD | Teff (K) | Kp | Δν (μHz) | νmax(μHz) | Star category | Duration (in months) | Quarters |
|
|
|||||||||
| 1435467 | – | – | 6433 ± 86 | 8.9 | 70.9 | 1324 | F-like | 24 | Q5-Q12 |
| 2837475 | – | – | 6688 ± 57 | 8.5 | 76.0 | 1522 | F-like | 24 | Q5-Q12 |
| 3424541 | – | – | 6475 ± 66 | 9.7 | 41.3 | 712 | F-like | 24 | Q5-Q12 |
| 3733735 | 94071 | 178971 | 6711 ± 66 | 8.4 | 92.4 | 2041 | F-like | 24 | Q5-Q12 |
| 6116048 | – | – | 6072 ± 49 | 8.4 | 100.7 | 2020 | simple | 24 | Q5-Q12 |
| 6508366 | – | – | 6499 ± 46 | 9.0 | 51.6 | 959 | F-like | 24 | Q5-Q12 |
| 6679371 | – | – | 6598 ± 59 | 8.7 | 50.4 | 908 | F-like | 24 | Q5-Q12 |
| 7103006 | – | – | 6421 ± 51 | 8.9 | 59.9 | 1072 | F-like | 24 | Q5-Q12 |
| 7206837 | – | – | 6392 ± 59 | 9.8 | 79.0 | 1556 | simple | 24 | Q5-Q12 |
| 8379927 | 97321 | 187160 | 6034 ± 74 | 7.0 | 120.4 | 2669 | simple | 24 | Q5-Q12 |
| 8694723 | – | – | 6351 ± 62 | 8.9 | 75.1 | 1384 | simple | 24 | Q5-Q12 |
| 9139151 | 92961 | – | 6134 ± 48 | 9.2 | 117.0 | 2610 | simple | 24 | Q5-Q12 |
| 9139163 | 92962 | – | 6405 ± 44 | 8.3 | 81.4 | 1649 | simple | 24 | Q5-Q12 |
| 9206432 | 93607 | – | 6494 ± 46 | 9.1 | 85.1 | 1822 | F-like | 24 | Q5-Q12a |
| 9812850 | – | – | 6407 ± 47 | 9.5 | 65.3 | 1186 | F-like | 24 | Q5-Q12 |
| 10162436 | 97992 | – | 6346 ± 108 | 8.6 | 55.9 | 1004 | simple | 24 | Q5-Q12b |
| 10355856 | – | – | 6558 ± 56 | 9.2 | 68.3 | 1210 | F-like | 15 | Q5-Q9c |
| 10454113 | 92983 | – | 6197 ± 45 | 8.6 | 105.2 | 2313 | simple | 24 | Q5-Q12 |
| 10909629 | – | – | 6501 ± 61 | 10.9 | 49.7 | 813 | F-like | 21 | Q5-Q11d |
| 11081729 | – | – | 6605 ± 51 | 9.0 | 90.2 | 1820 | F-like | 24 | Q5-Q12 |
| 12009504 | – | – | 6270 ± 61 | 9.3 | 88.1 | 1768 | simple | 24 | Q5-Q12 |
| 12258514 | 95568 | 183298 | 5990 ± 85 | 8.1 | 74.8 | 1449 | simple | 24 | Q5-Q12 |
| 12317678 | 97316 | – | 6549 ± 48 | 8.7 | 64.1 | 1162 | F-like | 24 | Q5-Q12 |
Notes. The first three columns provide the KIC, HIP, and HD numbers. The fourth column provides the effective temperature and its error bar from Pinsonneault et al. (2012). The fifth column provides the Kepler magnitude. The sixth column gives the median of the large separation as measured using the mode frequencies given in this paper. The seventh column provides the frequency of the maximum of oscillation power. The eighth column gives the star category as provided by Appourchaux et al. (2012a). The penultimate column gives the duration of observation. The last column provides the start and end quarters of the observation.
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