Rare Event Statistics Applied to Fast Radio Bursts

Abstract

Statistical interpretation of sparsely sampled event rates has become vital for new transient surveys, particularly those aimed at detecting fast radio bursts (FRBs). We provide an accessible reference for a number of simple, but critical, statistical questions relevant for current transient and FRB research and utilizing the negative binomial model for counts in which the count rate parameter is uncertain or randomly biased from one study to the next. We apply these methods to re-assess and update results from previous FRB surveys, finding as follows. 1) Thirteen FRBs detected across five high-Galactic-latitude (> 30${}^{\circ }$) surveys are highly significant $(p=5\times 10^{-5})$ evidence of a higher rate relative to the single FRB detected across four low-latitude (< 5${}^{\circ }$) surveys, even after accounting for effects that dampen Galactic plane sensitivity. High- vs. mid-latitude (5 to 15${}^{\circ }$) is marginally significant $(p=0.03)$. 2) A meta analysis of twelve heterogeneous surveys gives an FRB rate of 2866 sky${}^{-1}$ day${}^{-1}$ above 1 Jy at high Galactic latitude (95% confidence 1121 to 7328) and 285 sky${}^{-1}$ day${}^{-1}$ at low/mid latitudes (95% from 48 to 1701). 3) Using the Parkes HTRU high-latitude setup requires 193 observing hours to achieve 50% probability of detecting an FRB and 937 hours to achieve 95% probability, based on the ten detections of (Champion et al. 2016) and appropriately accounting for uncertainty in the unknown Poisson rate. 4) Two quick detections at Parkes from a small number of high-latitude fields (Ravi et al. 2015; Petroff et al. 2015) tentatively favor a look long survey style relative to the scan wide HTRU survey, but only at $p=0.07$ significance.

References in corpus (1)

• Limits on Fast Radio Bursts from Four Years of the V-FASTR Experiment

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