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