Table 4.
Galactocentric distances and velocities for the satellites in our sample.
| Satellite | dGC (kpc) | Vrad (km s−1) | Vtan (km s−1) | V3D (km s−1) |
|---|---|---|---|---|
| Col I | 185 | −27 ± 4 |  |
 |
| Horo II | 76 | 35 ± 9 |  |
 |
| Phx II | 80 | −42 ± 3 |  |
 |
| Ret III | 100 | 92 ± 9 |  |
 |
| Col I | 185 | −24 ± 4 |  |
 |
| Hor II | 76 | 19 ± 7 |  |
 |
| Phx II | 80 | −42 ± 4 |  |
 |
Notes. Column 1 shows the name, Col. 2 the object distance, and Cols. 3–5 give the radial, tangential, and 3D velocity, respectively. In the top part we provide the determinations from the full sample of members, and in the bottom part the determinations using the very likely members. We indicate in boldface our preferred value.
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