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Magnetar-powered Long Gamma-Ray Bursts and Connection to Superluminous Supernovae and Fast Radio Bursts

  • Authors: Yu-Qi Zhou, Shuang-Xi Yi, Yu-Peng Yang, Yan-Kun Qu, Ning Gai, Yanke Tang, Fa-Yin Wang

Yu-Qi Zhou et al 2026 The Astrophysical Journal Letters 1004 .

  • Provider: AAS Journals

Caption: Figure 4.

The Bp–P0 correlation for the GRB sample (assuming ηx = 0.5). The best-fit curve is represented by the red solid line, with its corresponding 1σ confidence interval indicated by the shaded region. Top: Bp–P0 correlation (left) and its corner plot (right) for GRBs with redshifts. Bottom: Bp–P0 correlation (left) and its corner plot (right) for all GRBs.

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