This article has 2 errata:
[https://doi.org/10.1051/0004-6361/202039217]
[https://doi.org/10.1051/0004-6361/201832698e]
Table C.4
Dwarf positions and velocities from the Sun, not corrected for the solar motion or the local standard of rest.
| Name | X[kpc] | Y [kpc] | Z[kpc] | U[km s−1] | V [km s−1] | W [km s−1] |
|---|---|---|---|---|---|---|
| Fornax |  |
 |
 |
 |
 |
 |
| Draco |  |
 |
 |
 |
 |
 |
| Carina |  |
 |
 |
 |
 |
 |
| Ursa Minor |  |
 |
 |
 |
 |
 |
| Sextans |  |
 |
 |
 |
 |
 |
| Leo I |  |
 |
 |
 |
 |
 |
| Leo II |  |
 |
 |
 |
 |
 |
| Sagittarius |  |
 |
 |
 |
 |
 |
| Sculptor |  |
 |
 |
 |
 |
 |
| Bootes I |  |
 |
 |
 |
 |
 |
| LMC |  |
 |
 |
 |
 |
 |
| SMC |  |
 |
 |
 |
 |
 |
Notes. Quoted values are medians, with errors that indicate uncertainties calculated from the 16th and 84th percentiles, and were obtained from Monte Carlo sampling the (statistical and our best estimates of the systematic) errors in the observables. The conventions are the same as for the globular clusters in Table C.3.
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