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Table B.3

Masses, ρ, θ, separations and gravitational binding energy of the systems identified in the sample of work.

WDS Discoverer code Star M (M⊙) ρ (arcsec) θ (deg) s (103 au) (1033 J)
Double systems
00016−0102 2MASS J00013688-0101441 0.22±0.02 0.74±0.10
WIS 1 SIPS J0000-0112 0.13±0.01 1135 234 68.4±0.2
01005−1923 HD 5911 1.32±0.13 20.6±2.9
SHY 392 HD 6103 1.24±0.12 1725 126 140.8±0.3
01066+1353 HD 6566 1.32±0.10 3.69±0.52
SHY 396 HD 5433a 1.02±0.10 11089 305 643.7±1.2
01134−3932 HD 7382 1.32±0.13 7.82±1.11
SHY 397 HD 7052 0.89±0.09 4472 209 264.6±0.5
01326−4944 HD 9544 1.89±0.19 61.1±8.6
SHY 405 HD 9378 1.49±0.15 1001 231 81.2±0.1
02022−4550 HD 12586 1.31±0.13 4.63±0.66
SHY 410 HD 12808 1.21±0.12 8496 10 605.0±0.8
02025−3849 2MASS J02022892-3849021b 0.32±0.03 0.72±0.11
WIS 48 2MASS J02004917-3848535 0.09±0.01 1166 270 69.3±2.7
02310+0823 G 4-24 0.64±0.06 2.09±0.30
GIC 32 G 73-59b 0.21±0.02 3096 278 111.5±0.1
05444−0528 HD 38273 1.35±0.13 6.97±0.99
SHY 489 HD 37546 1.27±0.13 5025 252 435.2±0.9
07069+5511 HD 53075 1.04±0.10 8.87±1.25
TOK 508 [SLS2012] PYC J07067±5537 0.44±0.04 1587 357 91.2±0.1
07113+3307 HD 54717 1.19±0.12 26.2±3.7
SHY 190 HD 54718 1.00±0.10 1790 182 80.2±0.1
07160+5759 NLTT 17578a 0.99±0.10 1.43±0.20
TOK 510 LSPM J0716±5827 0.15±0.01 1693 11 183.9±0.4
07329−5249 2MASS J07325350-5249077 0.68±0.07 1.58±0.22
WIS 141 2MASS J07325706-5229111 0.21±0.02 1197 1.6 157.9±0.2
08237−5519 HD 71257 1.41 ±0.14 9.04±1.28
SHY 526 HD 72143a 0.95±0.09 3442 133 261.0±0.3
08388−1315 HD 73583 0.71 ±0.07 1.90±0.27
SHY 201 BD-09 2535 0.69±0.07 14236 326 449.3±0.2
08480−3115 HD 75514a,b 1.33±0.13 20.3±2.9
SHY 529 HD 75269a 1.08±0.11 1585 225 125.6±2.3
09467+1632 BD±17 2130a 0.82±0.08 3.84±0.54
TOK 531 LP 428-36 0.29±0.03 1610 243 110.1±0.7
09568+0415 HD 86147 1.32±0.13 16.4±2.3
TOK 533 LSPM J0956±0441b 0.52±0.05 1619 359 74.0±0.2
10532−3006 HD 94375a 1.32±0.13 1.91 ±0.27
SHY 563 HD 94542a 1.19±0.12 17541 178 1439±3
11214+0638 HD 98697 1.37±0.14 12.2±1.7
TOK 544 LP 552-34 0.28±0.03 1136 271 55.3±0.1
11265+2031 HD 99419 1.03±0.10 6.95±0.98
TOK 546 Gaia DR3 3978588911076420736 0.31±0.03 1737 70 80.2±0.1
11455+4740 HD 102158 1.05±0.11 11.9±1.7
LEP 45 G 122-46 0.38±0.04 1178 72 60.3±0.1
12213−5012 HD 107440a 1.16±0.12 19.0±2.7
TOK 556 HD 107735a 1.08±0.11 1195 57 115.7±0.5
13305+2231 HD 117528 1.19±0.12 6.40±0.90
SHY 626 BD±22 2587 0.94±0.09 3650 183 307.4±0.4
15031−4618 CD-45 9610 0.67±0.07 17.4±2.5
WIS 280 L 334-33 0.41 ±0.04 1020 136 27.73±0.01
15120+0245 LP 562-9 0.41±0.04 2.17±0.31
WIS 281 LP 562-10 0.22±0.02 1136 1.1 71.56±0.08
15208+3129 HD 136654 1.27±0.13 27.3±3.9
LEP 74 AX CrB 0.88±0.09 1582 326 72.37±0.05
15226+3953 G 179-28 0.93±0.09 3.23±0.46
WIS 284 LP 222-69 0.24±0.02 1035 249 119.7±0.2
15356+7726 LSPMJ1535±7725 0.84±0.08 13.4±1.9
WIS 288 LP 22-358 0.70±0.07 1133 318 77.2±0.1
15408−3252 HD 139696a,b 0.79±0.08 3.04±0.43
SHY 278 CD-32 10820 0.62±0.06 9296 264 281.6±3.3
15488+4929 LSPM J1548±4928 0.12±0.01 0.29±0.04
WIS 295 LSPMJ1550±4921 0.11±0.01 1106 114 85.0±0.7
15590+1820 HD 143292a 1.29±0.13 4.87±0.69
SHY 691 HD 142899 1.19±0.12 7867 344 556.7±0.8
17127+3235 BD±32 2868 0.93±0.09 4.69±0.66
WIS 313 LSPMJ1711±3236 0.21±0.02 1046 273 73.6±0.4
17166+0325 HD 156287a 1.24±0.12 1.68±0.24
SHY 715 HD 159243 1.08±0.11 17154 61 1407±3
18496+1313 HD 229635 0.89±0.09 3.77±0.53
SHY 309 HD 229830 0.70±0.07 7650 161 288.8±0.2
18571+5143 HD 176341 1.35±0.14 4.24±0.60
SHY 749 BD±49 2879 1.17±0.12 7890 208 660.3±1.0
18597+1615 HD 176441a 1.21±0.12 20.2±2.9
TOK 622 LSPMJ1858±1613b 0.54±0.05 1264 267 57.2±0.1
19290−4952 HD 182857 0.88±0.09 3.81±0.54
SHY 319 HD 185112a 0.89±0.09 8677 47 359.4±0.2
20080−0041 64 Aql 1.00±0.27 35.4±5.0
SHY 325 HD 190873 0.99±0.10 1059 228 49.2±0.1
20124−1237 ξ Cap 1.27±0.13 42.9±6.1
TDT2085 LP 754-50 0.55±0.06 1021 194 28.83±0.03
20371+6122 HD 196903 1.37±0.14 9.76±1.38
SHY 780 HD 198662 1.20±0.12 5176 100 296.0±0.3
20404−3251 HD 196746a 1.23±0.12 7.82±1.11
SHY 781 HD 196189 1.15±0.11 3623 310 316.8±1.4
21009−4132 L 424-30 0.25±0.02 4.69±0.66
WIS 346 APMPM J2101-4125 0.21±0.02 1036 5.5 19.41±0.01
21066+8048 G 261-37 0.62±0.06 10.5±1.5
TOK 632 G 261-40 0.43±0.04 1286 53 44.52±0.03
21105+2227 HD 201670e 1.74±0.17 2.49±0.35
SHY 793 HD 198759 1.45±0.15 15684 262 1783±15
21190+2614 HD 203030 0.91±0.09 5.20±0.74
TOK 634 Gaia DR3 1846992067932879744d 0.22±0.02 1701 34 66.8±0.1
22175+2335 G 127-13b 0.42±0.04 3.32±0.47
GIC 179 G 127-14 0.42±0.04 2107 13 94.0±0.8
22378−0414 κ Aqr 2.55±0.13 10.8±1.5
TOK 640 Gaia DR3 2624935581540867200 0.20±0.02 1223 247 83.1 ±0.6
Triple systems
02062−4726 CD-48 554(A) 0.79±0.08 6.00±0.72
NSN 219 CD-48 554B 0.50±0.05 1.9 200 0.1702±0.0003
WIS 52 LEHPM 2187 0.27±0.03 1135 12 102.3±0.2
04346−3539 HD 29231 0.93±0.09
TOK 488 L 447-2 0.39±0.04 1632 125 45.89±0.02
WIS 108 UCAC3 109-11370b 0.27±0.03 1201 140 33.77±0.01
06536−3956 L 454-11b 0.37±0.04 9.43±0.99
SUB 2 WT 202 0.64±0.02 3565 247 89.0±0.4
SUB 2 WT 201 0.64±0.02 3596 248 89.8±0.4
07166−2319 HD 56578a 2.42±0.24
SHY 508 HD 57527a 1.92±0.19 12620 166 1340±6
Gaia DR3 5613164850183516544 0.35±0.03 11792 151 1253±6
08211+4021 BD±40 2030a 0.96±0.10 16.3±1.7
TOK 516 G 111-70 0.68±0.07 1624 308 98.5±0.1
Gaia DR3 914608342177083648 0.38±0.04 2.2 222 0.1343±0.0002
09150+3837 HD 79392a 1.44±0.14 19.0±3.3
TOK 525 Gaia DR3 812086579467748736 0.38±0.04 1047 242 56.76±0.07
DAM1575 Gaia DR3 812109085097488768 0.16±0.02 28 27 1.510±0.002
09487−2625 HD 85043Aa 1.27±0.13 42.1 ±7.3
I 205 HD 85043Ba 0.69±0.07 1.8 281 0.0756±0.0001
TOK 532 PM J09486-2644 0.58±0.06 1157 181 47.9±0.1
10289+3453 HD 90681 1.07±0.11 3.77±0.65
SHY 215 HD 92194 0.97±0.10 10588 134 52.0±0.6
… Gaia DR3 749786356557791744 0.08±0.01 14 207 0.674±0.001
11513+4516 Ross 916A 0.38±0.04 8.14±1.415
KPP3247 Ross 916B 0.37±0.04 1.4 281 0.0405±0.0001
WIS 193 G 176-59 0.20±0.02 1116 344 33.08±0.04
12416+1026 27 Vir 1.93±0.19 9.67±1.67
SHY 610 HD 111069a 1.04±0.10 5595 52 400.9±1.0
… Gaia DR3 3927438805519604352 0.19±0.02 41 77 2.93±0.01
13470+3833 HD 120164 2.42±0.29e 39.2±6.8
SHY 633 HD 119767 1.19±0.12 2084 296 191.1±0.9
S 654 BD±39 2679 1.14±0.11 71 237 6.55±0.03
13496+1301 HD 120510(Aab) 2.66±0.277 27.7±3.9
SHY 635 HD 120865 1.44±0.14 4337 153 244.8±0.3
14153+0308 HD 124757Aa 8.13±4.64
STF1819 HD 124757B 0.9 166 0.03729±0.0001
SHY 261 HD 126961 1.18±0.12 11923 96 491.7±1.6
14190−0636 ι Vira 1.810±0.001h 50.8±5.1
SHY 71/HDS016 HD 125354(Aab)a 1.20±0.12i 3423 129 75.4±0.5
14396−6050 α Cen A 1.11±0.01j 41.1±4.1
RHD 1 α Cen B 0.93±0.01j 15 222 0.0207±0.0001
LDS 494 Proxima Centauri 0.12±0.01 7960 212 10.71±0.02
15318−0204 HD 138370 1.18±0.12
SHY 677 HD 138159 0.98±0.10 2970 335 225.8±0.3
… Gaia DR3 4416092627948054400 0.18±0.02 2822 339 214.6±0.3
17415+4924 Wolf 1378b 0.82±0.08 3.58±0.62
WIS 321 LSPM J1741±4941 0.28±0.03 1079 346 137.0±2.1
… Gaia DR3 1367008242580377216 0.17±0.02 4.4 314 0.56±0.01
19235−6924 HD 180808(A)a 1.18±0.12 47.9±8.3
DON 957 HD 180808B 0.61±0.06 2.8 249 0.1668±0.0002
SHY 755 HD 181958a 1.49±0.15 1662 119 98.2±0.1
19476+0105 ENG 67 HD 187003(Aab)a 2.40±0.24 3.81±0.54
SHY 322 BD±00 4221 0.69±0.07 16426 263 767.7±0.8
20084+1503 G 143-33 1.18±0.12 3.40±0.98
LDS1033 G 143-27(Aab) 1.16±0.12 2188 269 709.7±4.6
21096−1122 v Aqr 2.01±0.11 42.3±6.4
TOK 633 Gaia DR3 6895305771635806208 0.42±0.04 1053 313 52.5±0.3
… Gaia DR3 6895305771635806464c 0.21±0.02 1055 313 52.5±0.3
22596−1246 … HD 217250(Aab) 0.90±0.09k 2.10±0.30
TOK 642 Gaia DR3 2603671950077707776 0.12±0.01 1365 262 87.5±0.1
23328−1651 HD 221503 0.67±0.07 3.00±0.42
SHY 110/… G 273-59(Aab)a 0.48±0.05 12958 190 188.4±0.1
23506+5412 HD 223582a 1.30±0.13 69.0±12.0
SHY 840 HD 223788 1.20±0.12 1098 77 60.1±0.1
ES 700 BD+53 3238B 0.67±0.07 15 35 0.804±0.001
Quadruple systems
01024+0504 HD 6101Aa g 53.5±5.4
HDS 135 HD 6101Ba 0.5 53 0.01083±0.00003
WNO 50 EGGR 7(Cab) 0.77±0.08 1276 88 28.7±0.1
02462+0536 HD 17250 1.16±0.12 …
TOK 651 HD 17163 1.60±0.16 3271 194 186.6±0.3
RAO 9 HD 17250B 0.47±0.05 1.9 254 0.108±0.002
TOK 651 ATO J041.4695+05.4898 0.51±0.05 494 222 28.18±0.04
05222+0524 … HD 35066(Aab)a 1.45±0.15 36.0±6.2
TOK 497 TYC 109-530-1 0.76±0.08 1326 119 82.0±0.6
STT 106 HD 35066Ba 0.76±0.08 9.5 40 0.584±0.004
06384+3945 BD+39 1687 0.78±0.08 …
TOK 502 LP 205-19 0.26±0.03 1261 68 78.0±0.1
… LP 205-22c 0.22±0.02 2227 69 137.7±0.2
… Gaia DR3 945027740109972224 0.11±0.01 2685 196 166.1±0.2
08447−5443 KEL 1/I 10/… δ Vel (Aabc) 6.18±0.04l 96.6±9.7
SHY 49 HD 76653 1.21±0.12 5534 100 136.7±1.4
11486+1417 BU 603 HD 102590(Aab)a 1.88±0.19 16.5±2.9
TOK 552 Gaia DR3 3923967883532679168 0.54±0.05 1778 306 119.9±0.8
… Gaia DR3 3923191426460144896 0.20±0.02 10 77 0.680±0.005
12317+1208 HD 109032 1.46±0.15 …
SHY 607 BD+13 2551 1.17±0.12 4215 46 448.1±1.5
… Gaia DR3 3907691061288324992 0.23±0.02 344 334 36.6±0.1
… Gaia DR3 3904562400951238144 0.20±0.02 2986 148 317.5±1.0
15330−0111 11 Ser 1.27±0.35m 3.08±0.62
SHY 678 HD 142011 1.21±0.12 17755 103 1483±7
… Gaia DR3 4403070145373483392 0.43±0.04 17758 103 1483±7
… Gaia DR3 4403070149671286272c 0.40±0.04 17758 103 1483±7
18143−4309 HD 166793 1.54±0.15 …
SHY 740 HD 166533 1.49±0.15 3231 345 334.3±1.1
… Gaia DR3 6721465492884350080 0.46±0.05 169 42 17.5±0.1
… Gaia DR3 6724532477492271104 0.46±0.05 2554 337 264.2±0.8
20154+6412 MLR 60 HD 193215(Aab) 1.07±0.11 …
SHY 772 BD+63 1588 0.85±0.09 5820 247 370.3±16.2
… G 262-11 0.41±0.04 7074 29 450.0±19.7
22220−3431 B 557 HD 210111(Aab) 1.90±0.19 11.5±2.3
SHY 805 HD 212025b 1.52±0.15 11176 117 878.7±2.4
SHY 802 HD 212035 1.50±0.15 11205 116 880.9±2.5
22455+1112 … HD 215243(Aab)a,b 1.37±0.14f 50.0±8.7
SHY 358 BD+10 4812Aa 0.73±0.07 1796 60 66.4±0.9
BU 711 BD+10 4812Ba 0.64±0.06 1797 59 66.4±0.9
22497+6612 ι Cep 1.55±0.20 …
SHY 359 HD 215588 1.23±0.12 29040 184 1061±5
… UCAC3 297-187960 0.35±0.03 29055 184 1061±5
… SDSS J230056.41+640815.5 0.50±0.10 8477 149 310.6±1.5
23309−5807 HD 221738a 1.86±0.19 14.0±2.4
SHY 833 HD 221252(AB) 1.12±0.11 5053 203 493.4±1.1
I 145 TYC 8838-832-2 0.99±0.10 5053 203 493.4±1.1
Quintuple systems
07294−1500 HD 59438Aa 1.29±0.13 71.2±1.4
STF1104 HD 59438Ba 1.00±0.10 1.8 37 0.0654±0.0001
TOK 391 LP 722-24 0.56±0.06 1073 343 39.14±0.03
STF1104/TOK 391 HD 59438C(ab)b 0.52±0.05 21 185 0.749±0.001
16278−0822 RST3949/… υ Oph(Aabc)a 2.28±0.12k …
TOK 603 HD 148300 0.88±0.09 775 202 33.3±1.3
SHY 287 HD 144660 0.80±0.08 18223 272 781.6±31.6
Sextuple systems
02315+0106 HD 15695 1.75±0.18 …
STF 274 BD+00 415B 1.63±0.16 13 220 1.422±0.005
SHY 422 HD 17000 1.14±0.11 12071 115 1273±4
… HD 16985 1.07±0.11 13373 234 1410±4
… Gaia DR3 2497835645142616192c 0.30±0.03 21691 109 2285±7
… Gaia DR3 2514005200579732608 0.20±0.02 10471 303 1104±3
03503−0131 HD 24098A 1.36±0.14 …
SHY 164 HD 22584a 0.80±0.08 11678 252 516.7±0.6
BU 401 HD 24098B 0.70±0.07 4.6 73 0.2031±0.0002
… UCAC4 438-004875 0.52±0.05 11687 252 517.1±0.6
… Gaia DR3 3250466403920143488 0.10±0.01 697 29 30.87±0.03
… Gaia DR3 3250466403923273088 0.19±0.02 696 29 30.84±0.03
20489−6847 HD 197569 1.81±0.18 …
SHY 782 HD 199760 1.27±0.13 4872 107 421.2±0.7
… Gaia DR3 6376446646807117312 0.41±0.04 2.7 232 0.2344±0.0004
… Gaia DR3 6374759136976638336 0.30±0.03 6776 219 585.8±0.9
… Gaia DR3 6375565697474377088 0.32±0.03 10914 108 943.3±1.5
… Gaia DR3 6376941667557429888 0.17±0.02 4716 21 407.8±0.7
Septuple systems
19507−5912 HD 188162 2.82±0.28 …
SHY 761/I 121 HD 186957(Aab) 2.52±0.25k 3138 250 283.4±2.9
SHY 759 HD 186810 1.79±0.18 3528 248 318.6±3.3
… Gaia DR3 6447086042643463936 0.43±0.04 609 143 55.0±0.6
… Gaia DR3 6447030135053741952c 0.36±0.04 3536 248 319.4±3.3
… Gaia DR3 6447128820517666944 0.26±0.03 1381 270 124.8±1.3
20599+4016 COU2431/LSC 1 HD 200077(Aa1a2bBab) 4.14±0.23n,o 99.7±23.5
LEP 98/HDS2989 G 210-44(Aab)a,b 0.67±0.07 1213 258 49.2±0.3

Notes. (a) Proper motion anomaly measured by Kervella et al. (2019), Brandt (2021) or both. (b) RUWE > 10; (c) Large σVr for its G magnitude; (d) Classified as a white dwarf candidate by Gentile Fusillo et al. (2019), it has instead absolute magnitudes and colours of an intermediate M dwarf; (e) da Silva et al. (2015); (f) Tokovinin (2014); (g) Dynamical mass (Malkov et al. 2012); (h) Gontcharov & Kiyaeva (2010); (i) Mitrofanova et al. (2021); (j) Pourbaix & Boffin (2016); (k) Kervella et al. (2019); (l) Eker et al. (2018); (m) Feuillet et al. (2016); (n) Tokovinin (2018); (o) Montes et al. (2018).

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