Fig. 3 from Strong Mg II Systems in Quasar and Gamma‐Ray Burst Spectra

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Strong Mg II Systems in Quasar and Gamma‐Ray Burst Spectra

Authors: Cristiano Porciani, Matteo Viel, and Simon J. Lilly

Porciani, Viel, & Lilly 2007 The Astrophysical Journal 659 218.

Provider: AAS Journals

Caption: Fig. 3.

Cumulative probability distribution of the Mg II equivalent widths along GRBs listed in P06b (solid histogram) compared with the fit for QSO absorbers given by Prochter et al. (2006a). The two distributions are compatible at the 95.7% confidence level in the Kolmogorov‐Smirnov sense.

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