Percentage of stellar particles, separated by their birth environment, located in the kinematically selected halo in the solar vicinity identified as being part of any significant cluster (>3σ) by the single-linkage method (upper panels). The lower panels show the similar quantity but considering only the particles that belong to clusters where their progenitor is the dominant contributor to a given clump. In all panels, the grey histograms indicate the contribution of each progenitor to the solar vicinity halo. Note: the second bar represent the value of all the accreted stellar particles grouped together.