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Quantifying Element Importance for Mass Recovery from Population III Supernova Yield Fits

  • Authors: Zhongyuan Zhang, Alexander P. Ji, Vinicius M. Placco, Sanjana Curtis

Zhongyuan Zhang et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 4.

Element-by-element perturbations of the baselines. (a) Medium baseline: ﹩\bar{d}﹩ versus atomic number Z when a single element is modified. The dashed line is the unmodified medium-baseline ﹩\bar{d}﹩. Purple circle markers indicate the element is removed from the baseline; orange square markers indicate an element is added to the baseline. Greater differences from the dashed line imply a larger effect on the metric. (b)–(d) Low (red), medium (blue), and high (green) coverage baselines: ﹩{\rm{\Delta }}\bar{d}=| {\bar{d}}_{\mathrm{modified}}-{\bar{d}}_{\mathrm{baseline}}| ﹩ versus Z. Horizontal dashed lines show the thresholds used to group elements into importance tiers. All results use 100 mocks per model and noise level σ = 0.2; ﹩\bar{d}﹩ is averaged over the 14 mixing values.

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