Table 3.
Orbital properties of objects in our sample.
| Satellite | peri(1.6)(kpc) | apo(1.6)(kpc) | ecc(1.6)(kpc) | peri(0.8)(kpc) | apo(0.8)(kpc) | ecc(0.8)(kpc) |
|---|---|---|---|---|---|---|
| AquII |
 |
 |
 |
 |
 |
 |
| BooI |
 |
 |
 |
 |
 |
 |
| BooII |
 |
 |
 |
 |
 |
 |
| CVenI |
 |
 |
 |
 |
 |
 |
| CVenII |
 |
 |
 |
 |
 |
 |
| CarI |
 |
 |
 |
 |
 |
 |
| CarII |
 |
 |
 |
 |
> 500 |
 |
| CarIII |
 |
 |
 |
 |
 |
 |
| CBerI |
 |
 |
 |
 |
 |
 |
| CraI |
 |
 |
 |
 |
 |
 |
| CraII |
 |
 |
 |
 |
 |
 |
| DraI |
 |
 |
 |
 |
 |
 |
| DraII |
 |
 |
 |
 |
 |
 |
| EriII |
 |
> 500 |
 |
 |
> 500 |
 |
| FnxI |
 |
 |
 |
 |
 |
 |
| GruI |
 |
 |
 |
 |
 |
 |
| HerI |
 |
 |
 |
 |
 |
 |
| HorI |
 |
 |
 |
 |
 |
 |
| HyaII |
 |
 |
 |
 |
 |
 |
| HyiI |
 |
 |
 |
 |
 |
 |
| LeoI |
 |
 |
 |
 |
> 500 |
 |
| LeoII |
 |
 |
 |
 |
 |
 |
| LeoIV |
 |
 |
 |
 |
 |
 |
| LeoV |
 |
 |
 |
 |
 |
 |
| PhxI |
 |
> 500 |
 |
 |
> 500 |
 |
| PisII |
 |
 |
 |
 |
 |
 |
| RetII |
 |
 |
 |
 |
 |
 |
| SgrI |
 |
 |
 |
 |
 |
 |
| SclI |
 |
 |
 |
 |
 |
 |
| Seg1 |
 |
 |
 |
 |
 |
 |
| Seg2 |
 |
 |
 |
 |
 |
 |
| SxtI |
 |
 |
 |
 |
 |
 |
| TriII |
 |
 |
 |
 |
 |
 |
| TucII |
 |
 |
 |
 |
 |
 |
| TucIII |
 |
 |
 |
 |
 |
 |
| UMaI |
 |
 |
 |
 |
 |
 |
| UMaII |
 |
 |
 |
 |
 |
 |
| UMiI |
 |
 |
 |
 |
 |
 |
| Wil1 |
 |
 |
 |
 |
 |
 |
Notes. Column 1 lists the object name; Cols. 2, 3, and 4 (Cols. 5, 6, 7) give the pericenter, apocenter, and eccentricity of the orbit around the Milky Way in the more (less) massive potential of the DM halo with virial mass 1.6 × 1012 M⊙ (0.8 × 1012 M⊙). When the value of ra minus 1σ is larger than 500 kpc, we only quote “ > 500 kpc” in the table.
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