Table C.1.
Orbital parameters and estimated stellar masses where sufficient data exists to model the orbits using ELC.
Star | # Obs. | ω | e | P | k1 | T0 | a sin i | f(m) | M1 | M2 | Ref. |
---|---|---|---|---|---|---|---|---|---|---|---|
# Lit. | (°) | (d) | (km/s) | (JD-2400000) | (109m) | (M⊙) | (M⊙) | (M⊙) | |||
HD 105671 | 1 | 244.46 ± | 0.138 ± 0.050 | 817.60 ± 95.75 | 0.75 | 60605.361 ± 284.127 | 111.94 | 3.2e-5 | 5.33 ± 0.75 | 0.34 ± 0.25 | |
6 | - - | - - | - - | - - | - - | - - | - - | 7.40 | - - | (6,7) | |
CD-62 1346 | 1 | 355.93 ± 11.97 | 0.340 ± 0.060 | 358.18 ± 2.72 | 2.31 | 59938.048 ± 15.724 | 70.76 | 3.9e-4 | 2.89 ± 0.87 | 0.50 ± 0.23 | |
12 | - - | - - | - - | - - | - - | - - | - - | - - | - - | - - | |
HD 50264 | 5 | 249.25 ± 8.37 | 0.011 ± 0.006 | 912.40 ± 0.38 | 9.52 | 49579.283 ±. 20.442 | 271.76 | 0.069 | 1.25 ± 0.89 | 0.66 ± 0.32 | |
11 | 230 | 0.091 | 909.90 | 9.52 | 49541 | - - | - - | 0.90 | 0.60 | (6) | |
HD 196673 | 1 | 116.19 ± 1.49 | 0.589 ± 0.016 | 7784.88 ± 75.12 | 3.58 | 51697.923 ± 77.760 | 1823.0 | 0.019 | 5.08 ± 0.32 | 1.05 ± 0.04 | |
79 | 116 | 0.590 | 7780.00 | 3.70 | 51698 | 314.0 | 0.020 | 5.00 | 1.10 | (4,6) | |
HD 104979 | 2 | 164.34 ± 9.59 | 0.075 ± 0.022 | 18189.37 ± 621.76 | 1.65 | 60297.864 ± 149.790 | 1466.92 | 0.008 | 2.99 ± 0.65 | 1.10 ± 0.34 | |
128 | - - | 0.080 | 19295.02 | - - | - - | - - | - - | 2.70 | 0.75 | (6) | |
HR CMa | 6 | 180.80* | 0.055 ± 0.020 | 457.32* | 6.79 | 47357.722 ± 55.167 | 180.13 | 0.014 | 1.87 ± 0.95 | 0.60 ± 0.15 | |
38 | - - | 0.013 | 457.40 | - - | - - | - - | 0.035 | 2.10 | 0.75 | (5,6,10) | |
PV UMa | 3 | 22.69 ± 2.10 | 0.110 ± 0.004 | 80.52 ± 0.001 | 8.48 | 55155.728 ± 0.061 | 32.48 | 0.005 | 2.20 ± 0.64 | 1.01 ± 0.10 | |
140 | - - | 0.090 | 80.00 | - - | - - | - - | 0.005 | 3.90 | 0.94 | (6,8,9) | |
HD 31487 | 1 | 246.02 ± 60.45 | 0.049 ± 0.008 | 1086.80 ± 72.23 | 7.86 | 49432.182 ± 123.928 | 255.57 | 0.060 | 1.95 ± 0.98 | 0.73 ± 0.33 | |
36 | 238 | 0.050 | 1066.40 | 7.00 | 45173 | - - | 0.038 | 3.40 | 1.59 | (4,5) | |
BD+41 2150 | 3 | 358.86 ± 1.60 | 0.057 ± 0.001 | 306.82 ± 2.04 | 10.78 | 56323.099 ± 1.822 | 187.69 | 0.040 | 1.69 ± 0.94 | 0.88 ± 0.31 | |
70 | 315 | 0.055 | 323.0 | 11.80 | 56114 | - - | - - | 1.27 | - - | (8,12,13,14,15) | |
HD 135148 | 11 | 261.04 ± 18.45 | 0.114 ± 0.020 | 1405.19 ± 2.78 | 4.87 | 47477.107 ± 67.530 | 496.36 | 0.016 | 2.72 ± 1.73 | 0.72 ± | 0.35 |
36 | 273 | 0.123 | 1416 | 4.79 | 47534 | - - | - - | 0.80 | 0.26 | (1) | |
HD 209621 | 1 | 15.66 ± 10.55 | 0.005 ± 0.005 | 407.81 ± 0.42 | 11.98 | 45877.766 ± 15.605 | 247.32 | 0.072 | 2.30 ± 1.10 | 1.15 ± 0.24 | |
27 | - - | 0.000 | 407.4 | 12.05 | 45858 | - - | - - | 3.60 | - - | (4,8,11,12,13) | |
BD+04 2466 | 2 | 319.91 ± 2.23 | 0.166 ± 0.022 | 4762.26 ± 20.12 | 5.53 | 59908.329 ± 12.918 | 1131.9 | 0.080 | 2.40 ± 1.20 | 1.18 ± | 0.21 |
42 | - - | - - | 4600 | - - | - - | - - | - - | - - | 1.10 | (11,16) |
Notes. Uncertainties in the parameters are taken from the widths of the posterior distributions after MCMC optimization. For each star, the first line are the results from our analysis and the second line are the data from the literature.
References(1)Carney et al. (2003) (2)Eker et al. (2008) (3)Fekel & Eitter (1989) (4)McClure & Woodsworth (1990) (5)Van der Swaelmen et al. (2017) (6)Jorissen et al. (2019) (7)Delgado Mena et al. (2019) (8)Escorza et al. (2017) (9)Katoh et al. (2013) (10)Udry et al. (1998) (11)Bisterzo et al. (2011) (12)Jorissen et al. (2016) (13)Escorza et al. (2020) (14)Platais et al. (2003) (15)Sperauskas et al. (2016) (16)Abate et al. (2015) (17)Fekel et al. (1999) (18)Griffin & Beggs (1991)
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