Fig. 5

Testing for the existence of the DoS. The behaviour of ℛ for each view of the MW, given by the Galactic longitude of the normal vector for each plane-fit. ℛ = Nin/Nout is the ratio of the number of satellites within 1.5 × Δmin (Δmin = 28.9 kpc), Nin, to those further away from the best-fit line, Nout, calculated for all 24 known satellites, as well as for the fits to the 11 classical and the 13 new satellites separately (taking their respective rms heights as the relevant Δmin). The disc-like distribution can be clearly seen as a strong peak close to lMW = 150°. Note that the position of the peaks are close to each other for both subsamples separately. This shows that the new satellite galaxies independently define the same DoS as the classical satellite galaxies.
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