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Table B.1

Spectroscopic orbital elements for all SB1 and SB2 systems studied in this work.

Star ID Period e ω K1 K2
value error value error value error value error
Main Alt. TIC (d) (degrees) (km s−1)
HERMES sample
BD+13 1880 BD+13 1880 TIC 186812530 3.677(2) 0.0f 0.0f 90f 0.0f 5.0 0.1 – –
BD+30 3184 BD+30 3184 TIC 23470753 4.237216(5) 0.20 0.01 121.9 5.1 82.7 1.2 116.8 3.2
BD+36 3317 BD+36 3317 TIC 237195907 4.302147(3) 0.0f 0.0f 90f 0.0f 82.93 0.03 127.3 0.1
BD+47 1906 BD+47 1906 TIC 253049152 1.3993(4) 0.0f 0.0f 90f 0.0f 20.1 0.5 213.6 3.2
BD+67 1049 BD+67 1049 TIC 219110814 3.5888926(6) 0.0f 0.0f 90f 0.0f 18.64 0.06 – –
HD 107379 HD 107379 TIC 148895442 3.595266(3) 0.0f 0.0f 90f 0.0f 14.9 0.8 76.4 0.6
EL CVn HD 116608 TIC 165371937 0.795624(8) 0.0f 0.0f 90f 0.0f 30.0 1.6 242.4 2.7
NO Dra HD 135437 TIC 202442974 2.738920(2) 0.02 0.04 217 11 77.8 0.5 154.9 3.0
HD 138305 HD 138305 TIC 368291074 3.498(3) 0.0f 0.0f 90f 0.0f 106.4 0.2 109.39 0.08
α CrB HD 139006 TIC 274945059 17.360(5) 0.3795 0.0002 314.7 0.8 37.1 1.3 98.5 0.8
HD 13970 HD 13970 TIC 264614791 3.508808(2) 0.0f 0.0f 90f 0.0f 117.1 1.4 188.2 4.3
HD 150781A HD 150781A TIC 349444267 7.457(5) 0.139 0.001 189.0 0.6 84.8 0.6 85.7 0.1
V920 Her HD 151972 TIC 143009538 6.926(3) 0.0f 0.0f 90f 0.0f 85.4 0.4 90.98 0.09
HD 158148 HD 158148 TIC 351701483 17.91032(2) 0.0f 0.0f 90f 0.0f 18.0 1.1 129.0 0.4
HD 160363 HD 160363 TIC 311433319 1.837710(2) 0.0f 0.0f 90f 0.0f 28.2 0.8 – –
HD 172133 HD 172133 TIC 8705972 3.598199(4) 0.0f 0.0f 90f 0.0f 43.97 0.04 – –
BH Dra HD 178001 TIC 377192659 1.8172380(2) 0.0f 0.0f 90f 0.0f 105.8 0.6 162.8 2.0
V2108 Cyg HD 191530 TIC 378395625 2.560339(1) 0.0f 0.0f 90f 0.0f 44.7 3.2 72.6 1.4
V1898 Cyg HD 200776 TIC 273173532 1.5131193(2) 0.0f 0.0f 90f 0.0f 54.6 1.5 293.0 1.4
V383 Cep HD 208106 TIC 410522328 1.4957437(3) 0.0f 0.0f 90f 0.0f 122.9 0.7 151.8 4.2
HD 208510 HD 208510 TIC 299494754 1.5970321(2) 0.0f 0.0f 90f 0.0f 68.0 6.1 243.7 5.6
AH Cep HD 216014 TIC 377506471 1.7747483(4) 0.0f 0.0f 90f 0.0f 230.1 2.0 277.1 3.9
V350 And HD 2189 TIC 58107375 1.7111454(2) 0.0f 0.0f 90f 0.0f 125.5 1.0 133.7 1.3
u Tau HD 23466 TIC 426588729 2.4245(9) 0.22 0.01 230 8 22.5 2.7 75.2 2.8
HD 234713 HD 234713 TIC 48087401 3.067219(3) 0.0f 0.0f 90f 0.0f 101.87 0.03 102.9 0.6
HD 237866 HD 237866 TIC 137905382 1.5238(4) 0.0f 0.0f 90f 0.0f 19.5 1.8 – –
HD 2460473 HD 246047 TIC 116331699 9.91493(2) 0.0f 0.0f 90f 0.0f 1.3 0.6 – –
IM Aur HD 33853 TIC 368180294 1.2472686(2) 0.0f 0.0f 90f 0.0f 67.8 0.6 285.8 1.0
HD 348568 HD 348568 TIC 342480862 11.727766(4) 0.0f 0.0f 90f 0.0f 23.8 2.0 131.3 3.8
HD 348725 HD 348725 TIC 342794723 1.531346(1) 0.0f 0.0f 90f 0.0f 115.4 2.5 143.9 3.1
HD 350685 HD 350685 TIC 392053854 2.873796(2) 0.0f 0.0f 90f 0.0f 34.1 2.9 – –
HD 37646 HD 37646 TIC 75507062 0.6726158(4) 0.0f 0.0f 90f 0.0f 28.7 0.1 – –
WW Aur HD 46052 TIC 172171873 2.525018(1) 0.0f 0.0f 90f 0.0f 117.53 0.02 124.59 0.04
V459 Aur HD 46552 TIC 172421004 1.0626466(7) 0.0f 0.0f 90f 0.0f 65.2 1.6 149.8 2.5
HD 47046 HD 47046 TIC 353759550 1.7166(6) 0.0f 0.0f 90f 0.0f 14.0 0.7 134.5 1.3
AW Cam HD 48049 TIC 456263109 0.77134620(7) 0.0f 0.0f 90f 0.0f 113.5 2.7 252.9 3.3
HD 63887 HD 63887 TIC 457101125 3.791285(3) 0.0f 0.0f 90f 0.0f 104.1 0.4 119.2 0.9
V766 Cas HD 8027 TIC 241017747 2.3296557(4) 0.09 0.02 232 17 129.9 1.0 154.4 8.5
HD 89601 HD 89601 TIC 150251466 12.388(7) 0.4207 0.0003 191.28 0.08 30.60 0.01 – –
V453 Cyg HD 227696 TIC 90349611 3.890(1) 0.027 0.002 151.3 11.3 173.7 1.0 221.4 1.0
NY Cep HD 217312 TIC 13389059 15.2884(2) 0.444 0.001 54.2 1.7 110.6 1.6 141.7 7.0
16 Lac HD 216916 TIC 129538133 12.097(1) 0.047 0.004 40.5 1.6 23.75 0.06 – –
V436 Per HD 11241 TIC 403625251 25.936(1) 0.373 0.009 109.5 1.0 94.1 1.8 99.9 1.0
RX Dra RX Dra TIC 377190161 3.876(1) 0.0f 0.0f 90f 0.0f 85.8 0.2 104.6 0.3
V1425 Cyg HD 202000 TIC 344456744 1.2523886(1) 0.0f 0.0f 90f 0.0f 143.8 1.3 218.4 2.2
V446 Cep HD 210478 TIC 335265326 3.808(1) 0.0150 0.0005 69.7 17.4 42.3 1.9 309.7 2.4
CM Lac HD 209147 TIC 331221558 1.6047(1) 0.0f 0.0f 90f 0.0f 121.0 0.2 155.3 0.8
V398 Lac HD 210180 TIC 326374705 5.406081(1) 0.23 0.01 233.6 7.5 90.7 1.5 139.3 2.6
V402 Lac HD 210405 TIC 468792279 3.7818043(8) 0.358 0.005 56.7 2.9 125.5 0.3 128.5 0.5
FEROS sample
HD 100737 HD100737 TIC 290391601 2.552548(2) 0.0f 0.0f 90f 0.0f 56.9 0.5 – –
HD 104233 HD104233 TIC 307687961 1.823975(1) 0.0f 0.0f 90f 0.0f 42.0 0.9 92.3 4.2
HD 1217761 HD121776 TIC 448375181 1.737896(1) 0.0f 0.0f 90f 0.0f 81.8 1.1 – –
HD 3003442 HD300344 TIC 274687574 2.7902916(3) – – – – – – – –
HD 304241 HD304241 TIC 451259413 2.730422(3) 0.0f 0.0f 90f 0.0f 84.6 1.3 – –
HD 309317 HD309317 TIC 306139502 2.257301(2) 0.0f 0.0f 90f 0.0f 34.5 0.3 78.7 1.4
AE Pic HD46792 TIC 150442264 2.9816923(9) 0.075 0.005 58.4 26.4 114.1 1.3 158.9 3.6
HD 523491 HD52349 TIC 80041531 2.775849(3) 0.37 0.01 312.6 7.3 54.8 0.6 – –
V386 Pup2 HD62738 TIC 175254818 1.649314(1) – – – – – – – –
HD 67025 HD67025 TIC 79935432 1.2823665(1) 0.0f 0.0f 90f 0.0f 147.4 1.9 173.7 2.7
HD 75872 HD75872 TIC 29216374 0.94508671(6) 0.0f 0.0f 90f 0.0f 45.9 1.0 – –
HD 82110 HD82110 TIC 438089724 1.8810195(2) 0.0f 0.0f 90f 0.0f 78.2 1.0 178.8 1.5
HD 84493 HD84493 TIC 363146191 6.8760(2) 0.0f 0.0f 90f 0.0f 29.20 0.06 – –
HD 91141 HD91141 TIC 457540424 2.3821886(4) 0.0f 0.0f 90f 0.0f 15.58 0.08 72.7 1.8
HD 91154 HD91154 TIC 457545293 3.6631544(5) 0.0f 0.0f 90f 0.0f 36.5 1.5 – –
CD-45 4393 TYC8151-937-1 TIC 141858108 2.0494343(2) 0.0f 0.0f 90f 0.0f 16.9 0.7 – –
CD-47 43643 TYC8155-1212-1 TIC 270844716 3.6580419(5) 0.0f 0.0f 90f 0.0f 1.58 0.09 – –
CD-56 1160 TYC8514-106-1 TIC 382044531 0.7903919(1) 0.0f 0.0f 90f 0.0f 65.7 1.5 155.6 2.2

The terms e, ω, and Ki stand for the eccentricity, time of periastron passage, and RV semi-amplitudes, respectively. Cases where eccentricity and argument of periastron were fixed to 0.0 and 90°, respectively, are indicated with the superscript ’f’. Orbital period values and their uncertainties have been adopted from Table A.1.

1 The star is classified as an SB2 system based on the visual inspection of the LSD profiles and/or original observed spectra; however, the SPD solution could only be obtained for the brighter primary component.

2 Same as above but no stable SPD solution could be obtained for either of the components.

3 Either an SB1 system with a low K semi-amplitude of about 1.5 km s−1 or a single star showing LPVs; the methods employed in this work do not favour any of these hypothesis.

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