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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 5.

Mapping between the fit quality metric ﹩\bar{d}﹩ and the fractional mass error δ = ∣(Mtrue − Mfit)/Mtrue∣. At the ﹩\bar{d}﹩ attained by 10 representative element sets (Fe-Peak, Low, Low+Ni, Even-Z, Mid, Mid+, Mid+N−O−K, High, High+, and All), scatter points show all δ values across the HW10 grid (16,800 models × 100 mocks =1.68 × 106 points per set). Symbols mark the 50th, 68th, 75th, and 90th percentile thresholds at each ﹩\bar{d}﹩, and the smooth curves are exponential fits to these thresholds. The 75th percentile curve is highlighted (thicker line) since it is used to compute δ75 in Figure 6.

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