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Modeling Gamma-Ray Burst Spectra with Convolutional Neural Networks: Fast-cooling Synchrotron Emission in a Decaying Magnetic Field

  • Authors: Jia-Ming Chen, Ke-Rui Zhu, Shan Chang, Zhao-Yang Peng, Yong-Gang Zheng, Li Zhang

Jia-Ming Chen et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 8.

Comparison between the empirical Band/CPL functions and the ME_FCSYN_CNN model. The top panel shows the temporal evolution of the low-energy photon index α obtained from the Band and CPL fits. The red dashed and blue dotted lines denote α = −2/3 and α = −3/2, respectively. The middle panel shows the evolution of the spectral peak energy Ep. The bottom panel shows the BIC values of the ME_FCSYN_CNN, Band, and CPL models. The gray curve in each panel shows the prompt-emission light curve for reference.

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