Using 116 CHIME baseband non-repeaters, the energy function is Schechter-like at low redshift, but the high-redshift slope and rate evolution are too uncertain to choose between star-formation and old-stellar progenitors.
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Deriving the Energy Function of Non-repeaters from CHIME/FRB Baseband Data
Using 116 CHIME baseband non-repeaters, the energy function is Schechter-like at low redshift, but the high-redshift slope and rate evolution are too uncertain to choose between star-formation and old-stellar progenitors.