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Signature of a Magnetar Central Engine from the Multiband Afterglow of GRB 151027A Associated with a Supernova

  • Authors: Liang-Jun Chen, Xiang-Gao Wang, Hou-Jun Lü, WeiKang Zheng, Daniel A. Perley, Da-Bin Lin, Yihan Wang, De-Feng Kong, You-Dong Hu, Jie Xia, S. Bradley Cenko, Hong-Bang Liu, Fei Xie, Jing Lü, En-Wei Liang, Bing Zhang, Alexei V. Filippenko

Liang-Jun Chen et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 3.

The EN(E) spectra of GRB 151027A. Data are shown for the optical (magenta), Swift/XRT (gray), Swift/BAT (cyan), Fermi/GBM NaI (black), and Fermi/GBM BGO (red). The model components include: CPL (dashed–dashed line), intrinsic PL from X-ray (blue dashed–dotted line), optical (magenta dashed–dotted line), BB (dotted), and composite best fit (solid line).

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