Fig. 2
Comparison of the cumulative brightness distributions of the host of our X-Shooter emission-line spectroscopy (XES) in blue against representative GRB host samples in black and olive lines (Hjorth et al. 2012; Vergani et al. 2015). In the top left of each panel, we show the K.S.-test p-value to reject the null-hypothesis that both samples are drawn from a similar parent distribution.
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