Same as in Fig. 7 but for the temperature-dependent fragmentation threshold and the Shu-infall model with a maximum R_C of roughly 10 au (top panels) and 100 au (lower panels). The results for the temperature-independent fragmentation threshold are qualitatively the same. White areas represent cases without any planetesimal production, while grey areas are cases where the planetesimal mass is between zero and two M_⊕.