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Table C.4

Model parameters from the Wilson-Devinney code

ID Porb/T0 q=M2M1$q = {{{M_2}} \over {{M_1}}}$ a γ e ω K i Teff Ω r L2L1( TESS )${{{L_2}} \over {{L_1}}}({\rm{ TESS }})$ 3
(days/BJD) (R) (km s–1) (deg) (km s–1) (deg) (K)
CG Scl p 11.0356853 0.7844(7) 25.472(13) –15.19 0.0341(4) 231.2 51.362(35) 89.88(10) 5740 20.236 0.05149(16) 0.1946(26) 0.015
s 2458363.4311 65.479(46) 4950 27.008 0.03033(10)
HD 27476 p 6.5054348 0.4835(12) 22.434(27) 18.25 0.0430(2) 337.8 56.88(13) 88.019(15) 10500 12.559 0.08298(10) 0.0941(19) 0.002
s 2459119.8884 117.65(17) 6192 12.559 0.04866(9)
AW Col p 10.317555 0.6655(9) 27.589(22) 28.46 0.5423(3) 322.5(a) 64.338(45) 89.863(31) 7800 20.019 0.05398(11) 0.1842(15) 0.013
s 2459305.7532 96.68(11) 5927 21.267 0.03519(14)
TYC 6511-1799-1 p 26.38190 1.0024(14) 52.911(43) 7.01 0.5031(4) 112.1(a) 58.771(62) 89.255(20) 6158 26.217 0.04133(19) 1.3046(60) –0.013
s 2458473.3390 58.631(54) 6278 23.939 0.04572(14)
BD+17 1832 p 7.158435 0.8264(13) 22.854(21) –21.07 0 - 72.986(28) 87.061(21) 8230 13.133 0.08128(16) 0.4252(32) 0.008
s 2457147.3399 88.32(14) 7298 14.396 0.06210(18) 0.3749(37)(b) 0.008(b)
TYC 266-718-1 p 35.02402 0.7875(3) 56.739(12) –2.50 0.0487(2) 245.6 36.151(10) 89.720(6) 6100 48.49 0.02098(3) 0.2804(45) 0.029
s 2456813.7893 45.905(15) 5314 56.42 0.01425(6) 0.2541(27)(b) 0.003(b)
HD 149946 p 23.309700 0.8049(11) 46.938(35) 9.40 0.0257(8) 259.1 45.435(30) 88.596(11) 6590 22.468 0.04623(23) 0.3064(27) –0.003
s 2456909.3638 56.446(70) 6526 31.974 0.02610(14) 0.3049(28)(b) –0.016(b)
HD 159246 p 5.2169237 0.9798(60) 22.841(71) –10.34 0 - 109.62(49) 89.524(31) 11000 10.662 0.10330(12) 0.9113(40)(b) 0.032(b)
s 2457705.6436 111.88(48) 10842 10.670 0.10119(33)
VZ PsA p 11.526969 0.4746(6) 33.218(29) 21.36 0.3179(2) 197.6(a) 49.481(35) 88.872(26) 9193 11.272 0.09459(11) 0.0455(7) –0.034
s 2459069.8788 104.26(13) 6230 15.734 0.03389(12)
HD 219869 p 6.0620410 0.8869(9) 18.027(10) 4.65 0.0052(9) 102.5 70.603(40) 86.725(32) 6440 11.961 0.09038(20) 0.4470(53) 0.008
s 2459452.9385 79.606(73) 6252 15.053 0.06340(29) 0.4357(58)(b) –0.006(b)

Notes. Quoted uncertainties are the standard errors from the Differential Corrections subroutine.

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 a system, the orbital eccentricity, the longitude of periastron, the radial velocity semiamplitude, the orbital inclination, the effective temperature, the Roche potential, the fractional radius R/a, the light ratio in the TESS band and the amount of third light in the TESS band.

(a) very slow apsidal motion detected - see details in Sect. 5.4.

(b) Kepler band

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