Table 8.
Model parameters from the Wilson-Devinney code.
| ID | Porb/T0 |
 |
a | γ | e | ω |
 |
K | i | Teff | Ω | r |
 |
l3 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (days/BJD) | (R⊙) | (km s−1) | (deg) | (deg year−1) | (km s−1) | (deg) | (K) | |||||||
| GW Eri p | 3.6586647(8) | 0.9906(19) | 15.272(15) | 32.32(13) | 0 | – | – | 104.51(14) | 83.933(51) | 8270 | 9.353(71) | 0.11971(101) | 0.9417 | 0.028(3) |
| s | 2459153.1534 | 32.32(13) | 105.49(15) | 8180(2) | 9.436(71) | 0.11760(98) | ||||||||
| HD 32129 p | 16.4120349(7) | 0.6945(7) | 37.407(26) | 4.867(15) | 0.4374(7) | 61.20(2) | 0.0042(4) | 52.546(31) | 88.797(12) | 6725 | 21.212(52) | 0.05006(13) | 0.1724 | 0.022(2) |
| s | 2459481.5181 | 5.370(10) | 75.656(68) | 5775(3) | 28.24(13) | 0.02640(13) | 0.1571 (a) | 0.009(4) (a) | ||||||
| UW LMi p | 3.87431667(14) | 0.9807(9) | 13.7086(63) | −33.930(24) | 0 | – | – | 88.480(49) | 86.621(44) | 5970 | 11.21(11) | 0.09778(100) | 0.8804 (b) | 0 (b) |
| s | 2450854.7741 | −33.897(26) | 90.223(65) | 5935(2) | 11.56(14) | 0.09300(118) | 0.8645 (c) | 0 (c) | ||||||
| QR Hya p | 5.0058710(4) | 0.9701(11) | 15.9370(87) | 10.534(18) | 0.0001(1) | 217(11) | – | 79.128(67) | 86.087(7) | 5880 | 13.383(39) | 0.08059(25) | 0.8378 | 0 |
| s | 2458559.4578 | 10.603(17) | 81.567(57) | 5801(2) | 13.873(58) | 0.07547(34) | ||||||||
| V788 Cen p | 4.96637676(9) | 0.7881(14) | 18.6193(18) | −18.700(18) | 0 | – | – | 82.918(51) | 82.821(41) | 7820 | 7.613(22) | 0.14682(49) | 0.3126 | 0.021(2) |
| s | 2458578.9929 | −18.919(24) | 105.21(17) | 7406(3) | 10.046(58) | 0.08821(58) | ||||||||
| V338 Vir p | 5.9853360(16) | 1.1586(11) | 19.6047(89) | 2.760(13) | 0 | – | – | 88.572(50) | 84.747(33) | 6582(3) | 13.952(84) | 0.07819(51) | 2.2116 (a) | 0 (a) |
| s | 2457228.4125 | 2.635(13) | 76.446(55) | 6425 | 10.535(38) | 0.12064(47) | ||||||||
| V963 Cen p | 15.269303(7) | 0.9945(7) | 33.463(30) | −30.450(13) | 0.4223(16) | 140.10(3) | 0.0065(5) | 60.920(35) | 87.255(32) | 5800 | 24.869(81) | 0.04320(15) | 0.9714 | −0.028(4) |
| s | 2459356.3465 | −30.448(12) | 61.257(24) | 5808(6) | 25.15(11) | 0.04248(20) | 0.9731 (b) | 0 (b) | ||||||
| LX Mus p | 11.750601(2) | 1.0082(3) | 30.2789(46) | −4.860(11) | 0.1975(2) | 148.59(6) | – | 66.708(15) | 87.603(10) | 6525 | 23.77(16) | 0.04442(28) | 1.0941 | 0 |
| s | 2459334.453 | −4.881(11) | 66.163(12) | 6556(2) | 23.11(12) | 0.04610(23) | ||||||||
| V362 Pav p | 2.7484368(5) | 0.4530(19) | 11.655(32) | −0.83(6) | 0.0014(4) | 283(16) | – | 66.555(81) | 84.304(35) | 8200 | 5.785(17) | 0.18817(61) | 0.0284 | −0.054(5) |
| s | 2458672.6411 | −0.06(25) | 146.93(58) | 4962(3) | 7.542(37) | 0.07231(44) | ||||||||
| CQ Ind p | 8.9737116(2) | 0.8896(5) | 24.3265(78) | −30.820(12) | 0.2764(5) | 89.66(1) | 0.0118(6) | 67.179(32) | 89.159(10) | 6440 | 18.489(46) | 0.05795(16) | 0.5460 | −0.006(3) |
| s | 2459046.259 | −30.568(11) | 75.515(25) | 6122(3) | 20.646(93) | 0.04632(23) |
Notes. Quoted uncertainties are the standard errors from the Differential Corrections subroutine combined with errors from Monte Carlo simulations with the JKTEBOP code ver. 34. In the ID column “p” refer to the primary and “s” to the secondary. The meaning of the columns are: the observed orbital period (and epoch of the primary eclipse T0 given below), the mass ratio, the total semimajor axis a = a1 + a2, the apparent systemic velocity of each component, the orbital eccentricity, the longitude of periastron, the rate of apsidal motion, the radial velocity semiamplitude, the orbital inclination, the effective temperature, the Roche potential, the fractional radius, the light ratio in the TESS band and the amount of third light in the TESS band.
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