Accretion history of the potentially habitable planet formed in run SPH06-cJS-pp0 (marked with superscript ¹ in Tables 3 and 4, and also illustrated in Fig. 6). It forms at ~1.1 au, with 1.2 M_⊕ and 24 O_⊕ of water. Besides the actual results with our SPH collision model (solid lines), hypothetical growth curves with synthetic PM, and also with added cumulative losses are plotted – both defined and discussed in the text (Sect. 6.3). The crosses mark the respective property of the other (second) body in collisions, besides the traced planet.