Relative detection rates of three surveys as a function of the source count slope, αin. Detection rates are normalised to the HTRU rate, using a Euclidean universe with standard candles (Simple population, left panel), and a cosmological population with a broad luminosity function (Complex population, right panel). The dotted line is computed analytically; the solid and dashed lines are the results of frbpoppy. The real detection rate per survey is given in the centre, with solid blocks denoting the 1σ Poissonian error bars (real population, centre).
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