maps of @Nidever2010.

Most of the debris, however, is close to the current position of the Clouds (grey squares indicate the observed positions of the LMC and SMC). Particles are colour coded in Fig. \[fig:aitoff\] by their Galactocentric distance (see color bar), which shows a clear gradient along the stream with distances reaching up to $300$ kpc, well beyond the virial radius of the main host.

For reference, we indicate the positions of all known Milky Way satellites in the figure as well. Red filled circles correspond to the “classical” (i.e., brighter than $M_v=-8$) dwarf spheroidal (dSph) companions of the Milky Way; open circles indicate the position of previously known, fainter satellites. We refer the interested reader to S11 for a discussion of the probability of association with the LMC of those satellites.

The recently-discovered dwarfs that are the focus of this paper are shown using black starred symbols in Fig. \[fig:aitoff\]. We include in this sample: (i) the dwarfs reported by @Koposov2015 from year-1 DES data [see also @Bechtol2015], (ii) the $6$ certain detections from year-2 DES data [@Drlica2015], and (iii) additional individual discoveries such as Hydra II [@Martin2015 Hy II], Horologium 2 [@Kim2015a Hor 2], Pegasus 3 [@Kim2015b 