Left panel: Cumulative accreted stellar mass as a function of the progenitors of each galaxy. Right panel: Cumulative sum of the accreted stellar mass located in the stellar halo as a function of the progenitors. We only show up to ten progenitors for the most massive dwarf galaxies, but some of them have even more. The threshold that marks 90% of the accreted mass is represented with a horizontal dashed line. We do not find a correlation between the number of significant progenitors and the stellar mass of the galaxies.