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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. 1.

Underlying number density of strong Mg II systems and the fraction of dusty absorbers that match the observed abundance of Mg II systems (solid line) and the observed fraction of absorbers along very reddened lines of sight (dashed line) in the SDSS. The dotted lines mark the 0, 1, 2, and 3 σ Poisson fluctuations for the observed density along GRBs.

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