Figure 2 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 2.

Left: light curves (connected lines) presented along with the E _p evolution (circles with error bars) of the long GRBs in our sample. Right: time-resolved E _p as a function of flux, along with the best-fit line for the E _p − F correlation for the long GRBs in our sample.

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