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Table A.1.

KIC IDs, pulsational (Nind and fmax) parameters, and binary and atmospheric (log Porb, Morph, Teff, e, and ω) parameters of the 93 detached eclipsing binary systems with g-mode pulsating components identified during our study.

KIC Nind fmax (d−1) log (Porb (d)) Morph Teff (K) e ω (rad) p modes References
2720354 44 0.64896 0.450454 0.46 6513 0.0614 1.640 GG19
3127817 26 0.23569 0.636201 0.48 6504 0.0502 4.777
3248332 22 0.46456 0.867091 0.2 6578 0.1183 5.063
3327980 15 0.06892 0.626445 0.44 7321 0.0205 1.635 Present GG19
3352751 19 0.28099 0.543504 0.5 7909 0.0949 1.507
3544694 28 0.22904 0.584975 0.29 6172 0.0126 1.600
3867593 ( * ), ( * *) 30 1.72913 1.865294 0.02 7037 Deb11; GG19; Li20a
4055765 26 0.88393 1.299551 0.1 6440 GG19
4067110 21 2.72055 0.584399 0.16 6499
4076952 13 0.08277 0.989502 0.38 6228 0.0448 1.159
4544587 37 2.01316 0.340265 0.49 8255 0.2765 5.738 Ham13; GG19
4862625 21 0.37870 1.301035 0.06 6149 0.1693 3.106
4931073 6 0.86196 1.430579 0.08 6453 0.4128 3.295
4932691 ( * ), ( * *) 42 0.98395 1.257968 0.1 7109 0.3797 3.215 Kju16; GG19; Li20a
5024292 23 0.32312 0.633573 0.37 6147 0.0424 1.293
5217733 27 2.42189 2.207506 0.03 9116 0.6162 2.564 GG19
5384802 32 0.54996 0.784124 0.17 6203 0.0276 4.699
5565486 ( * ), ( * *) 32 1.51263 0.451026 0.5 6471 0.01 4.781 Lur17; GG19; Li20a
5738698 16 0.15341 0.682034 0.41 6210 0.0546 4.723 Mat16
5817566 12 0.70518 0.924909 0.47 7994 0.0448 4.724 GG19
5961350 36 0.34766 0.721206 0.14 6869 0.1433 4.706
6063448 21 0.01944 1.880915 0.03 6416 0.4612 6.055 Present Lur17; GG19
6109688 30 1.11643 1.148812 0.18 6845 0.3255 4.923 Lur17; GG19
6145939 36 0.58596 1.249086 0.05 6090 0.5566 1.560 Lur17; GG19
6147122 45 0.92076 1.188971 0.06 7625 0.2085 1.722 Lur17
6279974 17 0.62126 −0.09406 0.43 6022 0.5023 1.700
6290382 ( * ), ( * *) 40 1.84985 0.78733 0.13 7016 0.6439 1.588 Present Li20a
6362386 22 0.16419 0.66204 0.32 6983 0.0851 4.677
6449358 39 0.14915 0.761687 0.31 7449 0.1078 1.594
6523216 16 0.17204 1.155735 0.19 6200 0.1473 1.259
6631721 22 0.35052 1.137932 0.07 6153
6766748 28 0.12518 0.845276 0.25 6601 0.0199 4.537
6805146 19 0.52379 1.13924 0.16 6214 0.1492 5.623 GG19
6889235 23 0.16027 0.715056 0.43 9288 0.0079 4.733 Row10; GG19
7025851 11 0.43586 0.670339 0.31 6054 0.0232 1.470
7107567 5 1.23518 −0.09012 0.5 6897 0.0047 1.860 Bra15
7422883 22 0.44354 1.057458 0.16 6639 0.0673 2.938 Deb11; GG19
7449844 36 1.36898 0.061535 0.46 6834 0.0954 4.625
7599004 4 0.33479 0.683308 0.18 6118 0.0942 4.738 Bra15
7831363 10 0.72129 0.449827 0.25 6072 0.0614 1.525
7970760 19 0.1133 0.883628 0.25 6172 0.0228 1.498
8019043 26 0.4941 0.297889 0.34 6396 0.0922 4.765
8098728 10 0.44224 1.3889 0.35 6404 0.1501 2.484
8112013 11 0.65894 0.252979 0.47 6350 0.0083 4.506
8193315 42 1.46676 0.418943 0.43 6457 0.0052 1.188 Present GG19
8196180 32 0.28453 0.564863 0.31 7114 0.1511 3.140 KV18
8197761 ( * ), ( * *) 35 1.02452 1.295313 0.07 7068 Sow17; Li19a; GG19; Li20a
8316503 22 0.19483 0.704608 0.25 6103 0.1097 6.220 Kju16
8488876 7 0.37705 0.763569 0.18 6957 0.1438 5.988
8504570 34 0.24792 0.602896 0.35 6874 0.0187 4.715 Present GG19
8560861 18 0.53515 1.504787 0.12 7647 0.0384 0.299 Bor14; GG19
8569819 ( * ), ( * *) 37 2.1631 1.319104 0.17 7137 0.4046 4.723 Present Kur15a; GG19; Li20a
8700506 15 0.4533 1.641452 0.04 6608 0.4835 0.968
8719419 27 0.74121 1.101243 0.07 6642 GG19
8823868 22 0.72297 1.377964 0.16 9751 0.0068 4.651 Row10; GG19
8878681 13 0.23271 0.397303 0.33 6504 0.0657 4.690
9048145 33 0.19838 0.93791 0.15 6484 0.0056 1.573
9236858 ( * *) 32 1.78603 0.404334 0.45 6510 0.0545 1.569 Present GG19; Li20a
9278021 14 0.6275 0.526271 0.19 6331 0.027 0.900
9392702 28 0.2244 0.592101 0.37 6170 0.0247 4.687
9552608 34 1.32136 0.966171 0.11 7906 0.3194 5.544 Lur17
9637299 67 0.53663 0.274721 0.44 6061 0.0316 1.536
9711751 33 0.59909 0.233377 0.49 6429 0 3.142
9850387 ( * ), ( * *) 34 0.84868 0.439096 0.47 6808 0.0046 1.604 Present GG19; Zha20; Li20a
9898364 55 1.47549 0.853235 0.11 7300
9911112 6 0.05405 0.368036 0.37 8750 0.042 4.745
9936698 10 0.15046 0.7568 0.27 6393 0.0496 1.523 Bra15
10028352 3 1.71287 0.142014 0.36 6191 0.6149 1.603
10156064 12 0.19744 0.686273 0.32 7424 0.031 1.532
10453521 8 0.34836 −0.63681 0.36 6541
10486425 ( * *) 45 1.31896 0.722207 0.25 7018 0.0109 1.494 AS14; Zha18; GG19; Li20a
10489521 22 0.27982 0.508463 0.38 6147 0.0396 1.555
10549576 35 0.81913 0.958538 0.2 7492 0.0669 4.655 Present Lur17
10659313 24 0.13946 1.183251 0.06 6167
10686876 27 0.17696 0.418041 0.45 7944 0.0044 4.522 Present
10920086 18 0.90127 0.506937 0.37 6478 0.8804 1.614
10937609 20 0.39576 0.410006 0.5 6016 0.0235 4.756
10987439 12 0.6158 1.028352 0.1 6182 0.0449 5.482 Hel19
11021252 24 0.31271 0.51444 0.22 6165 0.0036 4.538
11099351 24 0.42547 0.376204 0.29 9353 0.0407 4.710
11231334 30 0.68783 0.61883 0.44 6278 0.0266 4.775 Lur17
11252617 31 0.44401 0.651096 0.19 6089 0.0349 1.508
11285625 7 0.56747 1.033039 0.23 6882 0.0293 4.685 Deb13; GG19
11358392 20 1.01685 −0.00657 0.44 6195 0.0407 4.693
11359305 12 0.33875 1.454648 0.02 6101 0.4907 2.741
11671429 21 3.5045 2.051012 0.07 7363 0.4377 5.705 Present Uyt11; GG19
11817750 25 0.52841 0.989563 0.15 6930 0.0391 1.392 Lur17; GG19
11820830 ( * *) 11 0.90456 1.104892 0.08 7007 GG19; Li20a
11913071 31 0.22199 0.57378 0.37 8329 0.0035 2.120 KA17
11923819 20 1.84782 1.520608 0.07 7724 0.2912 2.670 Lur17; GG19
12167361 27 1.20897 1.680616 0 8017 Lur17; GG19
12405950 10 1.38396 0.548958 0.28 6808 0.1526 4.147
12470041 ( * *) 25 1.47773 1.166363 0.04 7290 GG19; Li20a

Notes. The second-to-last column of the table indicates whether p-mode frequencies were also observed in their frequency spectra, and the last column lists the truncated references to studies in which g modes were discovered or analysed in these systems. ( * )Period-spacing patterns were found during our pulsational screening process. ( * *)Period-spacing patterns were found by Li et al. (2020a).

References. AS14: Kahraman Aliçavus & Soydugan (2014); Bor14: Borkovits et al. (2014); Bra15: Bradley et al. (2015); Deb11: Debosscher et al. (2011); Deb13: Debosscher et al. (2013); GG19: Gaulme & Guzik (2019); Ham13: Hambleton et al. (2013); Hel19: Hełminiak et al. (2019); Kju16: Kjurkchieva et al. (2016); KA17: Kjurkchieva & Atanasova (2017); KV18: Kjurkchieva & Vasileva (2018); Kur15a: Kurtz et al. (2015b); Li19a: Li et al. (2019a); Li20a: Li et al. (2020a); Lur17: Lurie et al. (2017); Mat16: Matson et al. (2016); Row10: Rowe et al. (2010); Sow17: Sowicka et al. (2017); Uyt11: Uytterhoeven et al. (2011); Zha18: Zhang et al. (2018); Zha20: Zhang et al. (2020).

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