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A Unified Framework for 10 TeV to EeV Diffuse Neutrino Sky and KM3-230213A

  • Authors: Shiqi Yu, 世琦 于, B. Theodore Zhang, 兵 张

Shiqi Yu et al 2026 The Astrophysical Journal Letters 1002 .

  • Provider: AAS Journals

Caption: Figure 4.

Left: confidence contours of the joint spectral fitting parameters for the prompt phase. Crossing points indicate the medians of the post-burn-in MCMC samples, while dashed lines mark the 1σ HPD interval of the marginalized 1D posterior distribution; values and priors are provided in Table 1. Right: parameter space of isotropic gamma-ray luminosity (Lγ,iso) and redshift (z) consistent with Fermi-LAT upper limits under GRB 100316D configuration. Markers represent parameter points along the 95% confidence level boundary used to illustrate the predicted flux in Figure 3. Coordinates for these boundary samples are provided in the legend in the upper-right panel.

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