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First Light of Neutron Star Mergers: Off-axis Cocoon Cooling X-Ray Emission from Short Gamma-Ray Burst Jets

  • Authors: Jian-He Zheng, Wenbin Lu

Jian-He Zheng and Wenbin Lu 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 7.

The ﹩{E}_{{\rm{iso}}}^{{\rm{rad}}}﹩ vs. Epeak diagram. The blue solid and orange lines show the Amati relation for the SGRB (Type-I GRB) and LGRB (Type-II GRB) populations, adopted from Y. Liu et al. (2025). The dark- and light- shaded regions indicate the 1σ and 3σ confidence intervals, respectively. The magenta point marks GRB 170817A. Colors represent different models, while the circles (θv = 10∘), squares (θv = 20∘), diamonds (θv = 30∘), and stars (θv = 45∘) denote different viewing angles.

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