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Detection of 2 MeV Spectral Bump and ∼40 MeV Emission Line from GRB 221009A

  • Authors: Zhi-Qiang Ding, Zhenxia Zhang, Yanqiu Zhang, Rui-Ze Shi, Xinqiao Li, Zhuo Li, Zhenghua An, Shaolin Xiong, Roberto Battiston, Shuangnan Zhang, Hua Feng, Dali Zhang, Yanbing Xu, Ping Wang, Xiaoyun Zhao, Yuqian Ma, Hong Lu, Xiangyang Wen, Yongjie Zhang, Xuhui Shen, Shigeng Yuan, Siquan Yang, Rongxue Kang, Chao Zheng, Yan Huang, Wen Su, Shengli Liu, Hui Wang, Xiaohua Liang, Jinzhou Wang, Ke Gong, Xiaojing Liu, Yaqing Liu, Sheng Yang, Zeren Zhima, Jianping Huang, Wei Chu, Na Zhou, Roberto Iuppa, Francesco Maria Follega, Marco Cristoforetti, Wangchen Xue, Lu Wang, Jiaqi Zheng, Jiacong Liu, Chenwei Wang, Wenjun Tan, Zhenghang Yu, Shujie Li, Hao Hong

Zhi-Qiang Ding et al 2026 The Astrophysical Journal Letters 1012 .

  • Provider: AAS Journals

Caption: Figure F16.

Comprehensive sliding-window analysis of the spectral line evolution. (a) Temporal evolution of the central line energy (Eline), determined using a 9 s moving window with a 1 s step. Each colored point corresponds to a specific time interval, as defined in the legend. The black dashed line and orange shaded region represent the PL decay model, ﹩{E}_{{\rm{line}}}\propto {(t-{t}_{0})}^{-1.05}﹩, and its associated uncertainty, respectively. (b) Temporal evolution of the Gaussian line width (σline). The open diamonds denote intervals for which the relative line width was fixed at σline/Eline = 0.1, whereas the filled points represent free fits. The measurements from Y.-Q. Zhang et al. (2024) are shown in blue. (c) Evolution of the relative line width, σline/Eline. The horizontal dashed line marks σline/Eline = 0.1. (d) Temporal evolution of the emission line flux using the same sliding-window color scheme. The red dashed–dotted line denotes the fit to the sliding-window measurements, ﹩{F}_{{\rm{line}}}\propto {(t-{t}_{0})}^{1.86\pm 0.38}﹩, while the black dashed line and orange shaded region indicate the late-time decay model, ﹩{F}_{{\rm{line}}}\propto {(t-{t}_{0})}^{-2.16}﹩, and its associated uncertainty. Note: for the intervals from Tref + 237–246 through Tref + 240–249 s, the relative line width was fixed at σline/Eline = 0.1 because of the limited statistics. Beginning with the Tref + 241–250 s interval, all line parameters were allowed to vary freely.

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