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Pulse-resolved Classification and Characteristics of Long-duration Gamma-Ray Bursts with Swift-BAT Data. II. Main Bursts versus Extended Emissions

  • Authors: Liang Li, Xiao Wang, Zhi-Li Cui, Cheng-Long Xiao, Wen Li, Yu Wang, Zi-Gao Dai, Rong-Gen Cai

Liang Li et al 2026 The Astrophysical Journal Supplement Series 285 .

  • Provider: AAS Journals

Caption: Figure 4.

Duration–HR diagrams for the 24 analyzed GRBs in our sample. Each panel overlays the ME (G1, magenta star) and EE (G2, orange star) on the GRB population from A. Goldstein et al. (2017), color coded by Type I (short; black) and Type II (long; blue). The ellipses are used only as visual guides to the Type I and Type II regions. Both components lie in the long-GRB region, while G2 is usually displaced toward lower count hardness than G1.

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