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Table B.3.

Systemic proper motions obtained for the sub-set of systems analysed including the spectroscopic term for the likelihood.

Galaxy μα, *, sys μδ, sys fgal C P( > 0.5) P( > 0.8) P( > 0.95)
[mas yr−1] [mas yr−1]
AntliaII 0.18 1319 709 305
AquariusII −0.24 9 5 4
BootesI −0.14 199 163 134
BootesII −0.13 22 20 17
BootesIII 0.34 97 60 43
CanesVenaticiI 0.23 152 140 132
CanesVenaticiII 0.32 15 15 15
CarinaII −0.02 70 48 30
CarinaIII 0.02 12 11 9
ColumbaI −0.07 9 8 6
ComaBerenices −0.30 45 39 29
CraterI −0.24 13 13 12
CraterII −0.01 533 364 204
DracoII −0.04 29 25 21
EridanusII −0.20 20 19 18
GrusI 0.08 13 12 11
GrusII 0.28 38 27 21
Hercules 0.54 45 39 32
HorologiumI 0.03 18 16 15
HorologiumII −0.07 6 4 3
HydraII 0.04 21 16 14
HydrusI −0.00 119 94 63
LeoIV −0.19 8 8 6
LeoV −0.15 8 8 8
LeoT −0.37 8 7 7
PegasusIII −0.04 0 0 0
Phoenix −0.13 209 209 204
PhoenixII −0.44 11 11 10
PiscesII 0.24 2 2 2
ReticulumII −0.13 72 68 53
ReticulumIII 0.09 6 3 3
SagittariusII −0.06 73 67 58
Segue1 −0.40 25 19 17
Segue2 0.25 19 18 14
TriangulumII 0.27 16 14 11
TucanaII −0.32 40 30 22
TucanaIII −0.24 51 39 28
TucanaIV −0.12 15 10 9
TucanaV 0.22 4 3 3
UrsaMajorI −0.04 55 50 37
UrsaMajorII 0.09 64 37 25
Willman1 −0.16 11 11 10

Notes. The meaning of the columns is as in Tab. B.2.

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