Optimization of Radio Array Telescopes to Search for Fast RadioBursts

preprint2020arXivOpen access

Abstract

We present projected Fast Radio Burst detection rates from surveys carried out using a set of hypothetical close-packed array telescopes. The cost efficiency of such a survey falls at least as fast as the inverse square of the survey frequency. There is an optimum array element effective area in the range 0 to 25 m2\rm{m^2}. If the power law index of the FRB integrated source count versus fluence α=d lnR/d lnF>−1α= d ~ln R/d ~ln F > -1 the most cost effective telescope layout uses individual dipole elements, which provides an all-sky field of view. If α<−1α<-1 dish arrays are more cost effective.

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