Figure 3 from X-RAYING EXTENDED EMISSION AND RAPID DECAY OF SHORT GAMMA-RAY BURSTS

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X-RAYING EXTENDED EMISSION AND RAPID DECAY OF SHORT GAMMA-RAY BURSTS

Authors: Yasuaki Kagawa, Daisuke Yonetoku, Tatsuya Sawano, Asuka Toyanago, Takashi Nakamura, Keitaro Takahashi, Kazumi Kashiyama, and and Kunihito Ioka

2015 The Astrophysical Journal 811 4.

Provider: AAS Journals

Caption: Figure 3.

Reduced χ² distributions of the best-fit spectral model of the power law (square) and blackbody (circle) for time-resolved spectra of GRB 080503. The open and filled squares are the result of the power-law model for the WT and PC mode data, respectively. The open and filled circles are the same but for the blackbody model, respectively.

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