Integrated (−530 ≤ v_LSR [ km s^-1 ] ≤ −482) brightness temperature [ K km s^-1 ] map of the area toward Andromeda’s southeastern disk. The M 31-HVCs 1,2 and 5 discovered by Westmeier et al. (2008) in that radial velocity range are also detected by EBHIS, however the EBHIS column densities are lower by about 25%. These HVCs are below the applied 5 − σ threshold applied to the other maps. To demonstrate the baseline quality of the EBHIS standard data reduction the lower brightness temperature cut has been set to −0.5 K km s^-1.