Table 2.
Rotation and photospheric activity for primaries of detected binary systems.
KIC | Porb | e | Prot | Porb/Prot | Type | νmax | Δν | Sph | Ref. |
---|---|---|---|---|---|---|---|---|---|
[d] | [d] | [μHz] | [μHz] | [ppm] | |||||
4914923 | 99.24 ± 0.07 | 0.21 ± 0.01 | 24.5 ± 3.8 | 4.04 | ASB1 | 1825 ± 107 | 88.57 ± 2.46 | 125.3 ± 3.7 | [1] |
5516982 | 24.12 ± 0.02 | 0.42 ± 0.03 | 24.5 ± 2.0 | 0.98 | SB1 | 1699 ± 109 | 85.0 ± 1.91 | 134.0 ± 4.6 | [1] |
5696625 | 611.35 ± 7.2 | 0.28 ± 0.06 | 10.6 ± 1.3 | 57.89 | ABS1 | 696 ± 4 | 39.24 ± 3.22 | 105.1 ± 5.9 | [1] |
5814512 | 222.54 ± 1.34 | 0.42 ± 0.09 | 5.6 ± 0.7 | 39.39 | ORB | 995 ± 21 | 53.35 ± 1.66 | 82.5 ± 6.5 | [1] |
(h) 7206837 | 4.05 ± 0.0 | 0.0 ± 0.01 | 4.0 ± 0.3 | 1.0 | SB1 | 1645 ± 120 | 79.17 ± 1.76 | 234.2 ± 16.1 | [1] |
(b) 7668623 | 4.82 ± 0.0 | 0.01 ± 0.01 | 5.5 ± 0.4 | 0.88 | − | 822 ± 45 | 46.82 ± 1.51 | 843.1 ± 46.9 | [1] |
8016496 | 711.7 ± 11.52 | 0.25 ± 0.02 | 10.9 ± 0.8 | 65.23 | ASB1 | 1045 ± 29 | 53.99 ± 1.5 | 93.6 ± 5.3 | [1] |
8414062 | 791.36 ± 7.68 | 0.07 ± 0.02 | 11.0 ± 0.8 | 71.94 | ASB1 | 1100 ± 13 | 72.74 ± 2.27 | 104.2 ± 5.3 | [1] |
8677016 | 347.4 ± 4.32 | 0.16 ± 0.06 | 29.6 ± 2.5 | 11.74 | SB1 | 1882 ± 53 | 92.64 ± 2.37 | 78.5 ± 2.7 | [1] |
9025370 | 239.12 ± 0.45 | 0.27 ± 0.03 | 23.2 ± 3.5 | 10.3 | ORB | 3045 ± 75 | 131.43 ± 3.42 | 250.9 ± 6.5 | [1] |
9098294 | 20.1 ± 0.0 | 0.02 ± 0.01 | 19.9 ± 1.3 | 1.01 | SB1 | 2368 ± 102 | 110.0 ± 3.16 | 223.8 ± 7.0 | [1] |
9209245 | 22.92 ± 0.0 | 0.22 ± 0.02 | 22.6 ± 1.4 | 1.02 | SB1 | 1017 ± 19 | 53.86 ± 1.5 | 155.2 ± 5.3 | [1] |
9225600 | 343.75 ± 2.01 | 0.41 ± 0.06 | 9.0 ± 0.7 | 38.24 | ASB1 | 1192 ± 29 | 64.01 ± 1.77 | 32.7 ± 2.7 | [1] |
(f) 9328372 | 95.9 ± 0.58 | 0.28 ± 0.08 | 3.9 ± 0.7 | 24.47 | SB1 | 1379 ± 48 | 68.66 ± 1.82 | 307.2 ± 22.2 | [1] |
(c) 9390670 | 1041.87 ± 156.35 | 0.54 ± 0.26 | 3.6 ± 0.2 | 293.48 | SB1 | 1351 ± 26 | 71.07 ± 1.97 | 705.4 ± 49.1 | [1] |
9702369 | 195.76 ± 0.3 | 0.4 ± 0.02 | 11.6 ± 0.9 | 16.88 | ASB1 | 2039 ± 118 | 94.05 ± 2.36 | 50.5 ± 2.5 | [1] |
(e) 9898385 | 13.78 ± 0.01 | 0.01 ± 0.06 | 3.4 ± 0.3 | 4.1 | SB1 | 1352 ± 33 | 69.29 ± 1.92 | 368.9 ± 27.5 | [1] |
(g) 10355856 | 4.49 ± 0.0 | 0.0 ± 0.01 | 4.5 ± 0.3 | 1.0 | SB1 | 1320 ± 79 | 67.41 ± 1.31 | 299.8 ± 19.6 | [1] |
(a) 10775748 | 6.48 ± 0.0 | 0.01 ± 0.01 | 6.4 ± 0.5 | 1.01 | SB1 | 997 ± 10 | 60.88 ± 1.82 | 843.2 ± 43.8 | [1] |
11862497 | 598.79 ± 7.41 | 0.66 ± 0.06 | 4.6 ± 0.4 | 129.89 | ORB | 1888 ± 47 | 90.7 ± 2.09 | 88.6 ± 7.0 | [1] |
12317678 | 80.84 ± 0.06 | 0.39 ± 0.04 | 3.7 ± 0.7 | 21.97 | ORB | 1244 ± 79 | 63.49 ± 1.18 | 51.4 ± 4.2 | [1] |
3942719 | 339.26 ± 1.41 | 0.24 ± 0.04 | 38.0 ± 5.0 | 8.94 | ASB1 | 788 ± 27 | 45.2 ± 1.66 | 532.8 ± 6.45 | [2] |
3952580 | 45.74 ± 0.02 | 0.34 ± 0.01 | 89.8 ± 7.6 | 0.51 | SB1 | 636 ± 22 | 37.09 ± 1.11 | 140.6 ± 1.16 | [2] |
6587236 | 688.01 ± 17.57 | 0.05 ± 0.09 | 17.9 ± 2.2 | 38.46 | ASB1 | 499 ± 2 | 32.09 ± 1.57 | 89.8 ± 2.28 | [2] |
8408931 | 18.57 ± 0.0 | 0.1 ± 0.01 | 18.4 ± 1.3 | 1.01 | SB1 | 609 ± 4 | 33.98 ± 1.54 | 192.34 ± 3.4 | [2] |
(d) 9163769 | 3.17 ± 0.0 | 0.01 ± 0.02 | 3.2 ± 0.2 | 1.0 | SB1 | 1573 ± 11 | 80.62 ± 1.88 | 451.47 ± 17.89 | [2] |
10732098 | 199.15 ± 0.46 | 0.65 ± 0.03 | 25.6 ± 6.0 | 7.79 | ASB1 | 1055 ± 42 | 60.11 ± 1.85 | 85.65 ± 1.76 | [2] |
11709205 | 57.9 ± 0.02 | 0.41 ± 0.01 | 58.0 ± 3.3 | 1.0 | SB1 | 271 ± 12 | 18.95 ± 0.87 | 224.65 ± 2.28 | [2] |
3437031 | 623.74 ± 10.24 | 0.08 ± 0.07 | 138.8 ± 7.2 | 4.49 | ASB1 | 63 ± 3 | 5.6 ± 0.18 | − | [3] |
4358067 | 139.5 ± 0.58 | 0.34 ± 0.06 | 67.5 ± 4.4 | 2.07 | ASB1 | 4 ± 0 | 0.71 ± 0.04 | − | [3] |
4758020 | 290.39 ± 6.41 | 0.18 ± 0.18 | 124.2 ± 4.7 | 2.34 | SB1 | 92 ± 6 | 7.5 ± 0.14 | − | [3] |
5087190 | 959.44 ± 106.84 | 0.33 ± 0.15 | 66.1 ± 9.5 | 14.51 | SB1 | 70 ± 3 | 6.08 ± 0.13 | − | [3] |
5382824 | 653.29 ± 4.31 | 0.11 ± 0.02 | 92.2 ± 7.9 | 7.08 | SB1 | 100 ± 4 | 8.0 ± 0.23 | − | [3], [4] |
5439339 | 98.04 ± 0.07 | 0.03 ± 0.02 | 60.4 ± 5.3 | 1.62 | SB1 | 99 ± 5 | 7.89 ± 0.28 | − | [3], [4] |
5534910 | 851.96 ± 38.35 | 0.24 ± 0.11 | 94.8 ± 6.7 | 8.99 | SB1 | 112 ± 5 | 8.26 ± 0.24 | − | [3] |
5707338 | 885.17 ± 14.19 | 0.27 ± 0.07 | 60.4 ± 4.3 | 14.65 | SB1 | 81 ± 4 | 6.49 ± 0.18 | − | [3] |
6032639 | 979.76 ± 45.02 | 0.29 ± 0.07 | 123.4 ± 4.1 | 7.94 | SB1 | 46 ± 2 | 4.73 ± 0.15 | − | [3], [4] |
6933666 | 48.34 ± 0.11 | 0.18 ± 0.08 | 99.2 ± 2.6 | 0.49 | SB1 | 34 ± 2 | 3.83 ± 0.12 | − | [3], [4] |
7661609 | 106.58 ± 0.08 | 0.19 ± 0.01 | 104.6 ± 3.1 | 1.02 | SB1 | 23 ± 1 | 2.7 ± 0.4 | − | [3] |
8365782 | 702.84 ± 5.19 | 0.07 ± 0.02 | 116.0 ± 4.1 | 6.06 | SB1 | 81 ± 3 | 6.3 ± 0.13 | − | [3] |
8825444 | 128.52 ± 0.21 | 0.04 ± 0.02 | 83.7 ± 7.6 | 1.54 | SB1 | 83 ± 4 | 6.57 ± 0.15 | − | [3] |
8936339 | 796.03 ± 54.97 | 0.05 ± 0.12 | 103.2 ± 5.0 | 7.71 | SB1 | 44 ± 2 | 4.62 ± 0.62 | − | [3] |
9086060 | 453.2 ± 11.43 | 0.21 ± 0.09 | 81.0 ± 4.0 | 5.59 | SB1 | 48 ± 2 | 4.77 ± 0.16 | − | [3] |
9240941 | 254.08 ± 1.04 | 0.13 ± 0.04 | 125.2 ± 6.3 | 2.03 | SB1 | 110 ± 5 | 8.34 ± 0.18 | − | [3] |
9469212 | 992.55 ± 141.7 | 0.26 ± 0.14 | 68.4 ± 6.7 | 14.5 | SB1 | 45 ± 2 | 4.31 ± 0.12 | − | [3] |
9898373 | 617.06 ± 16.97 | 0.05 ± 0.08 | 128.6 ± 6.8 | 4.8 | SB1 | 45 ± 3 | 4.73 ± 0.63 | − | [3] |
10148118 | 388.24 ± 2.65 | 0.06 ± 0.03 | 89.7 ± 9.1 | 4.33 | SB1 | 62 ± 3 | 5.46 ± 0.19 | − | [3] |
10935853 | 882.61 ± 17.57 | 0.3 ± 0.07 | 62.6 ± 5.6 | 14.11 | SB1 | 65 ± 3 | 5.76 ± 0.13 | − | [3] |
11650041 | 107.17 ± 0.29 | 0.04 ± 0.05 | 53.0 ± 7.9 | 2.02 | SB1 | 8 ± 0 | 1.41 ± 3.07 | − | [3] |
12314910 | 69.53 ± 0.06 | 0.02 ± 0.02 | 104.5 ± 3.7 | 0.67 | SB1 | 24 ± 1 | 2.91 ± 0.08 | − | [3], [4] |
Notes. The star’s identifier in the Kepler input catalog is given in the first column. The next columns report the period Porb and eccentricity e of the orbit as reported in the Gaia DR3 TBO catalog. The next column corresponds to the period of the surface rotation Prot of the primary, determined from the light curve analysis. Porb/Prot reports the ratio between the orbital and rotation period, whereby Porb/Prot = 1 suggests that orbit and surface rotation are synchronized. The next three columns give the global seismic parameters of the power excess and large frequency separation as well as the photospheric activity indicator Sph. The last column reports the main references for the target, where Aerts (2021) refers [1] to Santos et al. (2021), [2] to García et al. (2014a), [3] to Ceillier et al. (2017), and [4] to Beck et al. (2022).
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.