Fig. 11

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Redshift distribution of BNSs through detection of GWs and sGRBs. In blue, we show the distribution for ET. Again, in orange, we plot the distribution of Fermi/GBM GRBs (same distribution as Figs. 10, 12 and 13), where the red region corresponds to the off-axis GRBs, generated with the addition to our model as described in Sect. 3.4. The orange region with dotted line represents those GRBs with a peak flux between 50 and 100% of the Fermi/GBM detection threshold.
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