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Table 1.

Properties of 15 eclipsing binary systems with eccentric orbits, accurate absolute dimensions, and literature-predicted relativistic apsidal motion relative contribution greater than 60%.

System Ps [d] e M1 [M] M2 [M] R1 [R] R2 [R] Refs.
KX Cnc 31.2197874(14) 0.4666(3) 1.138(3) 1.131(3) 1.064(2) 1.049(2) 99 Sow12
AL Dor 14.90537(2) 0.1952(2) 1.1029(4) 1.1018(5) 1.121(10) 1.118(10) 98 G&G
RW Lac 10.369205(2) 0.0098(10) 0.928(6) 0.870(4) 1.186(4) 0.964(4) 96 Lac05
V530 Ori 6.1107784(3) 0.0880(2) 1.004(7) 0.596(2) 0.980(13) 0.587(7) 92 Tor14
HP Dra 10.7615(2) 0.0367(9) 1.133(5) 1.094(7) 1.371(12) 1.052(10) 89 Mil10
TZ Men 8.569000(10) 0.035(3) 2.49(3) 1.504(10) 2.02(2) 1.432(15) 86 And87
V541 Cyg 15.3378992(7) 0.4684(14) 2.335(17) 2.260(16) 1.859(12) 1.808(15) 86 Tor17
LV Her 18.435954(2) 0.6127(7) 1.193(10) 1.170(8) 1.358(12) 1.313(11) 83 Tor09
V459 Cas 8.45825381(19) 0.0244(4) 2.02(3) 1.96(3) 2.009(13) 1.965(13) 80 Lac04
RR Lyn 9.94508(6) 0.0793(9) 1.927(8) 1.507(4) 2.57(2) 1.59(3) 80 Tom06
V501 Her 8.5976870(10) 0.0956(8) 1.269(4) 1.211(3) 2.002(3) 1.511(3) 78 Lac14
KW Hya 7.750469(6) 0.094(4) 1.96(3) 1.487(13) 2.124(15) 1.44(2) 77 G&A
V501 Mon 7.0212077(10) 0.1339(6) 1.646(4) 1.459(3) 1.89(3) 1.59(3) 71 Tor15
GG Ori 6.6314936(17) 0.2218(22) 2.342(16) 2.338(17) 1.85(3) 1.83(3) 67 Tor00
EY Cep 7.971488(6) 0.4429(14) 1.523(8) 1.498(14) 1.463(10) 1.468(10) 64 Lac06

Notes. Only systems with primary and secondary eclipse coverage from the TESS mission are considered.

References. Sow12: Sowell et al. (2012); G&G: Gallenne et al. (2019) and Graczyk et al. (2019); Lac05: Lacy et al. (2005); Tor14: Torres et al. (2014); Mil10: Milone et al. (2010); And87: Andersen et al. (1987); Tor17: Torres et al. (2017); Tor09: Torres et al. (2009); Lac04: Lacy et al. (2004); Tom06: Tomkin & Fekel (2006); Lac14: Sandberg Lacy & Fekel (2014); G&A: Gallenne et al. (2019) and Andersen & Vaz (1984); Tor15: Torres et al. (2015); Tor00: Torres et al. (2000); Lac06: Lacy et al. (2006).

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