Fig. 7
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Impact of progenitor mass on the supernova yields as compared to the best-fitting model. Three-dimensional non-LTE abundances from this paper are shown as red squares together with the best-fitting progenitor supernova model in blue and three other models with a higher progenitor mass in grey: M = 50, 70, 100 M⊙, E51 = 0.3 and fmix = 0.25.
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