Abundance patterns of light (30 ≤ Z < 55; left panel) and heavy neutron-capture elements (55 ≤ Z ≤ 92; right panel). The colored points represent derived abundances for the ten sample stars. The abundances for each star were rescaled by subtracting the mean offset from HD 222925 (Roederer et al. 2018). The pattern of HD 222925 is represented by the solid gray line and dots; upper limits are indicated with gray downward facing triangles. The lower panel displays the residuals with respect to the reference star HD 222925. The dashed gray line is the solar r-process pattern from Sneden et al. (2008).