Fig. 1.
Left panel: distribution of observable FRB host galaxies with total flux above 10 μJy at 1.4 GHz per square degree per redshift, dngal(z)/dz, binned in redshift bins of 0.1 width taken from the SKA Simulated Skies. Middle panel: distribution of potentially observable FRBs from these host galaxies per square degree per year, assuming an internal emission rate of Rint = 10−4 per galaxy per day. Right panel: integrated number of observable FRBs per square degree per year from z to zlim = 6.
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