Table A.3
Light curve and orbital solutions for our targets.
| Parameter | LSI+61 145 | AN Dor | TYC 1881-933-1 | HD 254346 | TYC 741-1565-1 | HD 309317 | HD 112485 | HD 350685 | HD 154407C | VI208 Sco |
|---|---|---|---|---|---|---|---|---|---|---|
| M1(M⊙)-fixed | 11.2 | 8.2 | 6.6 | 11 | 8.8 | 9 | 11.6 | 11.2 | 11 | 13.12 |
 (K)-fixed |
26000 | 21529 | 18700 | 24757 | 23634 | 22978 | 26096 | 25832 | 25696 | 29600 |
| P(d)-fixed | 1.846333 | 2.032883 | 1.019711 | 5.431772 | 2.257173 | 2.257341 | 5.372445 | 2.873794 | 2.558821 | 5.219670 |
| γ(kms−1) | −36.5±1.9 | 54.9±2.0 | 15.1 ±0.4 | 11.9±2.5 | 44.3±1.6 | −10.3±1.4 | −19.3±2.2 | 20.8±3.0 | 20.3±1.9 | −26.5± 0.3 |
| K1 (km s−1) | 22.2±2.8 | 59.6±2.8 | 38.7±0.5 | 15.6±3.8 | 8.7±2.2 | 25.6±2.0 | 55.0±2.8 | 32.3±5.3 | 13.2±2.2 | 44.7±0.4 |
| f(m) (M⊙) | 0.00209±0.00079 | 0.0444±0.0063 | 0.00612±0.00024 | 0.00213±0.00155 | 0.000153±0.000117 | 0.00393±0.00093 | 0.0923±0.0139 | 0.0100±0.0049 | 0.00060±0.00035 | 0.0483±0.0013 |
| e-fixed | 0 | 0.052 | 0 | 0.015 | 0 | 0 | 0 | 0 | 0 | 0 |
| ω(°) | 340.76(fixed) | 130.8±1.0 | ||||||||
| i(°) | 81.5±0.05 | 75.90±0.06 | 68.07±0.20 | 76.74±0.10 | 73.17±0.10 | 77.60±0.10 | 78.53±0.15 | 72.70±0.25 | 79.14±0.20 | 85.37±0.20 |
| q-fixed | 0.060 | 0.205 | 0.113 | 0.062 | 0.027 | 0.082 | 0.234 | 0.108 | 0.040 | 0.172 |
| M2(M⊙)-fixed | 0.67 | 1.68 | 0.75 | 0.68 | 0.24 | 0.74 | 2.71 | 1.21 | 0.44 | 2.26 |
| f1 | 0.569±0.004 | 0.676±0.005 | 0.792±0.003 | 0.416±0.001 | 0.602±0.001 | 0.561 ±0.001 | 0.412±0.003 | 0.458±0.007 | 0.454±0.007 | 0.359±0.003 |
| f2 | 0.517±0.001 | 0.601 ±0.005 | 0.780±0.002 | 0.239±0.001 | 0.422±0.001 | 0.431 ±0.003 | 0.289±0.011 | 0.751 ±0.006 | 0.463±0.010 | 0.300±0.005 |
| R1(R⊙) | 4.631 ±0.032 | 4.521 ±0.032 | 3.468±0.014 | 6.803±0.015 | 5.441 ±0.008 | 4.742±0.008 | 6.141 ±0.042 | 4.782±0.070 | 4.704±0.073 | 5.632±0.047 |
| R2(R⊙) | 1.221 ±0.002 | 1.948±0.016 | 1.293±0.003 | 1.140±0.005 | 0.808±0.002 | 1.195±0.008 | 2.206±0.080 | 2.912±0.023 | 1.178±0.025 | 2.108±0.035 |
 (K) |
8082-10286±500 | 9071-9941 ±150 | 8671-9826± 120 | 11680-12327±50 | 8295-10319± 175 | 7777-9430±150 | 13625-14017± 100 | 8074-9536±150 | 14214-14784±300 | 12252-12951 ±400 |
| Prot (d) | 2.12±0.03 | 1.37±0.01 | 1.14±0.17 | 1.67 ±0.02 | 1.77 ±0.07 | 1.15±0.01 | 1.66±0.08 | 0.93±0.02 | 1.61 ±0.09 | 3.27±0.30 |
| log(g1) | 4.16±0.01 | 4.04±0.01 | 4.18±0.01 | 3.81±0.01 | 3.91 ±0.01 | 4.04±0.01 | 3.93±0.01 | 4.13±0.01 | 4.43± | 4.05±0.01 |
| log(g2) | 4.09±0.01 | 4.08±0.01 | 4.09±0.01 | 4.16±0.01 | 4.00±0.01 | 4.15±0.01 | 4.18±0.03 | 3.59±0.01 | 3.94±0.02 | 4.14±0.01 |
Notes. The RV solution for AN Dor comes from Table 1 and that of V1208 Sco from Banyard et al. (2022) - see text for details. For the other targets, the zero point γ and amplitude K1 were calculated assuming zero eccentricity with the period and To from Table A.2. To calculate the photometric solutions of all targets, we fixed the eccentricities and ephemerides (Table A.2), primary masses and primary effective temperatures (from Table A.1), and mass ratios (derived from the mass functions f(m) and a preliminary fitting to get inclinations i). For secondary temperatures, the first value provides the usual effective temperatine (i.e., without any reflection effect) while the second value corresponds to a mean over the stellar surface, that is, it accounts for the heating of some parts of the star because of the reflection effect. The rotation period Prot is calculated using 2πR1 sin(i)/νsin(i).
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