Fig. 29

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Redshift and fluence for the FRBs presented here compared against those in the TNS (http://www.wis-tns.org) also detected in or before 2019. In this semi-log plot, a spectral index of -0.4 is used to compare the CHIME bursts (blue abscissa) with the other bursts (black abscissa). The Apertif FRBs are positioned around the midpoint of the 1.4 GHz FRB fluence distribution.
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