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Fig. 10.

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Δ(ReM) as a function of the redshift for GRB host galaxies. The orange and red circles are GRB hosts at z ≲ 1 from Kelly et al. (2014) and Blanchard et al. (2016), respectively. The blue circles are the GRB hosts considered in this study. Dark GRBs are highlighted by a thick black circle. The gray squares are the median of the Δ(ReM) for each redshift bin. The associated error bars are the standard deviation using the MAD estimator. The black line at y = 0 represents the expected median values for a GRB hosts population that do not suffer from environment bias.

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