Mass spectra with varying cloud bulk temperature. The colors blue, orange, green, red, purple, and brown represent the time at which about 20, 50, 100, 150, 200, and 300 M_⊙ have been accreted onto sink particles. Lognormal fits are shown with thin lines for reference. Top panel: canonical run T10M0+ (run C++ in Paper I), where the non-magnetized run has an EOS that sets the low-density gas to T₀ = 10 K. Middle panel: (T40) with T₀ = 40 K, similar peak position as the canonical run. Bottom panel: (T100) with T₀ = 100 K, same characteristic peak mass, while the formation of low-mass sinks is clearly more difficult.