Using one dataset and multiple damping wing models, the authors trace earlier conflicting GRB 130606A neutral fraction results to modeling assumptions and derive a 3-sigma upper limit of x_HI < 0.20-0.23.
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Revisiting the Intergalactic Medium Around GRB 130606A and Constraints on the Epoch of Reionization
Using one dataset and multiple damping wing models, the authors trace earlier conflicting GRB 130606A neutral fraction results to modeling assumptions and derive a 3-sigma upper limit of x_HI < 0.20-0.23.