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arXiv:1604.03909 [astro-ph.HE]AbstractReferencesReviewsResources

The Euclidean distribution of Fast Radio Bursts

Niels Oppermann, Liam Connor, Ue-Li Pen

Published 2016-04-13Version 1

We investigate whether current data on the distribution of observed flux densities of Fast Radio Bursts (FRBs) are consistent with a constant source density in Euclidean space. We use the number of FRBs detected in two surveys with different characteristics along with the observed signal-to-noise ratios of the detected FRBs in a formalism similar to a V/V_max-test to constrain the distribution of flux densities. We find consistency between the data and a Euclidean distribution. Any extension of this model is therefore not data-driven and needs to be motivated separately. As a byproduct we also obtain new improved limits for the FRB rate at 1.4 GHz, which had not been constrained in this way before.

Comments: five short pages; comments welcome
Categories: astro-ph.HE, astro-ph.IM
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