High-z gamma-ray burst detection by SVOM/ECLAIRs: Impact of instrumental biases on the bursts’ measured properties

Open Access

Fig. 3.

Rest-frame T₉₀ as a function of redshift for the GRBs in the sample, colour-coded based on the bursts E_iso. The solid line corresponds to the $T_{90}^{src}$ ${T_{90}^{\mathrm{src}}}$ rolling average up to z ∼ 5 computed in z-bins of unity size, spaced by 0.4 in redshift.

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