Integrated column density map (−600 km s^-1 ≤ v_LSR ≤ −95 km s^-1) of the HI emission in between M 31 and M 33. All HI emission displayed exceeds the applied 5σ threshold of the EBHIS data. The crosses mark the location of the known HI clouds at systemic velocities (Wolfe et al. 2013). The systemic velocity clouds V and VI closely match the lower velocity clouds in position, while the others are offset by a few degrees. The low-velocity cloud population shows up as a single filament with a pronounced core-halo structure.