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Table C.1

Statistics of solution 0 < G < 10.5 for each star

Star v Qi / vi Ei Ωi
(mas−2) (mas−2 yr2)
SY Scl 5 4.65 0.0 93.8
S Per 5 24.82 0.0 43.7
LS I +61 303 7 11.78 22.2 5082.8
HD 22468 7 11.59 20.3 1435.6
V410 Tau 7 12.05 412.4 2725.2
HD 283572 12 1.54 73.8 4719.7
V1110 Tau 5 3.36 28.3 446.5
HD 282630 5 12.62 47.2 147.0
V1321 Ori 5 0.70 33.6 86.1
V1046 Ori 5 4.53 7.2 136.4
HD 37150 5 3.46 7.5 261.1
HD 290862 5 0.97 2.4 16.2
VY CMa 5 26.17 0.0 14.9
BH CVn 9 3.49 27.5 868.6
S CrB 3 7.19 0.0 27.4
U Her 3 4.70 0.0 20.6
RR Aql 3 18.76 0.0 5.1
Cyg X-1 10 1.60 13.4 4747.5
HD 199178 12 0.96 36.0 4232.6
AR Lac 14 3.08 153.7 3794.5
IM Peg 12 6.25 23.2 505.1
PZ Cas 5 18.14 0.2 53.3
UV Psc 2 0.17 12.9 207.4
HD 8357 7 5.14 13.3 460.0
RZ Cas 7 1.45 39.9 968.3
SV Cam 2 0.60 13.8 222.2
54 Cam 2 0.40 12.3 197.4
IL Hya 2 4.24 11.4 183.0
DK Dra 2 6.79 11.3 181.9
RS CVn 7 0.47 99.4 5050.1
del Lib 4 11.06 1.0 16.3
V1859 Ori 5 3.47 32.2 2591.0
AR Mon 4 0.47 57.2 1898.8
XY UMa 5 0.59 41.3 1113.0
DM UMa 5 0.93 40.6 3097.9
RS UMi 5 3.74 49.4 5551.0
HD 179094 5 0.51 1.3 36.1

Notes. v is the total VLBI data dimension of each star, e.g., 5 for five-parameter measurement and 2 for one-epoch measurement. Qi / vi is the normalized loss. Ei and Ωi are weights (amounts of information contributed) in orientation and spin respectively. Only accepted stars are listed in this table.

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