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Table 6

Results from jktebop fits to light curves (detached systems only) and approximate stellar parameters, assuming primary is TeffA = 7500 K.

Renson RB/RA i e JB/JA P T eff B R A R B q q (literature)
3750 0.307 0.111 89.95 0.00 0.00 1.2199 2000§ 1.63 0.18 0.07 <0.003 (Collier Cameron et al. 2010)
4660 0.298 0.910 87.61 0.00 0.84 2.7807 7176 1.97 1.80 0.92 0.91 (Southworth et al. 2011)
6720 0.344 1.354 79.59 0.00 0.91 2.3832 7333 1.68 2.26 1.07
7310 0.161 0.601 86.37 0.00 0.50 6.6637 6322 2.20 1.32 0.71
7730 0.156 3.000 89.57 0.24 0.10 39.2827 4218 2.93 8.71 0.84 0.96 (Popper 1988)
8215 0.105 0.940 86.43 0.00 0.44 8.7959 6126 1.38 1.29 0.77
9237 0.248 1.036 80.52 0.00 0.49 2.8562 6288 1.51 1.55 0.81
9318 0.148 0.472 85.89 0.06 0.72 11.1133 6901 3.24 1.52 0.71
9410 0.189 0.634 87.74 0.02 0.30 16.7873 5537 5.07 3.19 0.59 0.81† (Lucy & Sweeney 1971)
10016 0.242 1.323 86.98 0.25 1.03 5.4309 7557 2.11 2.81 1.11
11100 0.165 0.397 85.07 0.00 0.36 4.0375 5818 1.79 0.71 0.61
11470 0.228 0.580 89.36 0.00 0.39 2.8721 5931 1.75 1.02 0.66
14850 0.215 0.272 83.02 0.00 0.08 3.9795 3925 2.43 0.66 0.30
15034 0.202 0.469 83.88 0.00 0.54 7.5392 6423 3.39 1.59 0.65
15190 0.174 0.439 82.60 0.00 0.02 5.1229 2952 1.97 0.86 0.21 0.33† (Carquillat et al. 2003)
15445 0.270 0.881 86.32 0.00 0.92 5.7606 7355 3.10 2.72 0.93
21400 0.106 0.513 86.63 0.00 0.04 7.7729 3435 1.49 0.77 0.29
22860 0.136 0.558 83.84 0.28 2.81 7.9006 9712 2.33 1.30 1.17
25020 0.188 0.081 89.10 0.00 0.00 6.6284 2000§ 3.39 0.28 0.06
25070 0.185 0.500 85.60 0.14 0.91 6.7149 7323 2.85 1.42 0.79 1.00 (this work)
29290 0.314 0.977 79.45 0.00 0.95 3.2922 7406 2.30 2.23 0.98
30090 0.221 0.788 82.26 0.00 0.97 4.3486 7451 2.11 1.67 0.93
30110 0.148 0.162 84.55 0.00 0.09 4.3145 4108 1.92 0.31 0.37
30457 0.137 0.231 86.82 0.00 0.00 11.9420 2000§ 3.20 0.74 0.08
30650 0.060 0.378 88.38 0.00 0.00 18.1210 2000§ 1.53 0.58 0.09
35000 0.190 0.835 82.07 0.00 0.00 10.2861 2000§ 2.69 2.26 0.13
36660 0.096 0.698 88.61 0.41 0.71 16.3653 6892 2.30 1.60 0.81 0.80 (this work)
37220 0.135 0.962 85.57 0.00 0.97 5.7931 7437 1.38 1.33 0.98
37610 0.240 1.455 85.50 0.00 1.28 3.2387 7974 1.38 2.02 1.19
38500 0.173 0.348 83.65 0.00 0.19 3.9938 4945 1.87 0.65 0.47
40350 0.156 0.272 88.22 0.00 0.00 7.0687 2000§ 2.43 0.66 0.08
40910 0.132 1.114 87.17 0.05 1.05 11.1163 7594 2.03 2.23 1.05
42906 0.062 0.860 87.84 0.00 0.00 19.6987 2000§ 1.23 1.06 0.12 0.98 (Carquillat et al. 2003)
44140 0.309 1.391 86.51 0.02 0.66 2.0598 6763 1.31 1.81 0.96 0.90 (Popper 1970)
49380 0.161 0.355 85.06 0.11 0.57 5.0204 6508 2.14 0.76 0.68 0.83 (this work)
51506 0.322 0.119 80.30 0.12 0.17 1.9196 4787 2.69 0.32 0.46 0.12 (this work)
56310 0.285 1.108 84.26 0.00 0.88 2.6959 7258 1.68 1.85 0.99
58170 0.366 0.854 88.24 0.00 0.48 1.6047 6246 1.65 1.42 0.77 0.78 (Popper 1968)
58256 0.271 0.378 81.63 0.00 0.41 2.9673 5983 2.50 0.95 0.59
59780 0.228 1.200 87.87 0.33 0.95 7.3514 7412 2.61 3.15 1.06 0.98 (Torres et al. 1999)

Notes. See text for details.

(†)

Mass ratio (q) obtained using spectroscopic binary mass function, f(m), and assuming M1 = 1.7 M⊙ and i = 90.

(§)

Lower-limit on TeffB imposed when JB/JA = 0.

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