Fig. C.1.
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Marginalized posterior of the sn parameter for Set A (top row) and Set B (bottom row) and for the three considered star temperatures, namely T = 108K (left panels),T = 109K (central panels) and T = 1010K (right panels). We show the results for the three assumptions on the threshold “Always” (MdUrca < 1.3 M⊙), “Sometimes” (1.3 M⊙ ≤ MdUrca ≤ 2.1 M⊙) and “Never” (MdUrca > 2.1 M⊙) (blue dotted, orange dashed and green dash-dotted, respectively).
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