Mollweide projection of the Galactocentric coordinates (Φ_gc, Θ_gc). The projection is divided into a grid of 48 pixels (nside = 2) with equal area. The blue, red, yellow, and orange regions delineate the regions associated with VOD, HAC-N, HAC-S, and Pisces at their typical distances. Top panel: the inner slope, α_in, measured at r_q = 15 kpc, of the two power law model. Middle panel: the outer slope, α_out, measured at r_q = 50 kpc, of the two power law model. Bottom panel: the difference between α_in and α_out. These panels highlight the anisotropy of the MW stellar halo profile, where several patches of the sky have distinct slopes compared to the average halo. We only show patches with more than four density points in the radial binning. The crosses and “x” indicate the regions with |α_out|−|α_in|< 1.5, and |α_out|−|α_in|> 1.5 with error in the break radius greater than 25%, respectively.