Abundance distribution integrated over the whole outer crust for an initially cold NS of mass 1.5 M_⊙ and 13 km radius. The distributions are arbitrarily normalized to the solar system r-abundance distribution, shown for comparison. The distributions are obtained with the HFB-19 (squares), HFB-21 (circles) and D1M (diamonds) mass models when experimental masses (Audi et al. 2003, 2010) are not available.