  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.
