Figure 4 from A Comprehensive Analysis of Fermi Gamma-Ray Burst Data. II. E p Evolution Patterns and Implications for the Observed Spectrum-Luminosity Relations

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A Comprehensive Analysis of Fermi Gamma-Ray Burst Data. II. E p Evolution Patterns and Implications for the Observed Spectrum-Luminosity Relations

Authors: Rui-Jing Lu, Jun-Jie Wei, En-Wei Liang, Bin-Bin Zhang, Hou-Jun Lü, Lian-Zhong Lü, Wei-Hua Lei, and Bing Zhang

Lu et al. 2012 The Astrophysical Journal 756 112.

Provider: AAS Journals

Caption: Figure 4.

Comparison of time-resolved Band spectral parameters, i.e., (a) low-energy spectral index, (b) peak energy, and (c) high-energy spectral index, between the 350 bright CGRO/BATSE GRBs with 8459 time-resolved burst spectra (gray shapes; Data from Kaneko et al. 2006) and the Fermi GRBs included in our sample (solid lines).

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