Left: the map shows the column density distribution of the Hi 21-cm line emission across the velocity interval −80   km   s^-1 ≤ v_GSR ≤ 250   km   s^-1. The complex Hi structure is produced by the superposition of the Milky Way galaxy emission, the LMC, and the LA. Right: the column density distribution of LA clouds across −80   km   s^-1 ≤ v_GSR ≤ 250   km   s^-1 starting at a threshold of ΔT_B = 200   mK (4-σ level of the GASS data). All the objects shown are cataloged and parametrized. Coherent structures like the Milky Way disk and LMC emission are according to the applied criteria “border” objects and not part of the catalog. The boxed and labeled areas enclose coherent structures in the data cube. Objects outside these areas also belong most likely to the LA. Note: white colors inside regions with disk emission denote column densities in excess of N_HI = 9 × 10²²   cm^-2.