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Fast X-Ray Transients Produced by Off-axis Jet Cocoons from Long Gamma-Ray Bursts

  • Authors: Jian-He Zheng, Wenbin Lu

Jian-He Zheng and Wenbin Lu 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 9.

The Eiso versus Epeak diagram. The blue solid line represents the Amati relation for the LGRB population, taken from Y. Liu et al. (2025). The deep blue and light blue shaded regions indicate 1σ and 3σ uncertainties, respectively. The yellow (Lc), red (Lw), green (LI), and purple (Llow) are results in different models, while the circles (θv = 10°), squares (θv = 20°), diamonds (θv = 45°), and stars (θv = 60°) denote different viewing angles. Magenta points denote observed FXTs (EP240414a and EP250108a), for which Epeak only has upper limits.

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