SEA,RCH TECHNIQUES AND RESULTSA rntrnightf,)rward nmrrh rnttatr~y Fmpl;Iym the" l)lnnin~nflhe ;ky rnpntirdly, according to th~angular rmoluti(jn~)f thr nrray, where u is the angular resolution of the detector, For the case with no a prsoti source location (using the qvents in the data set to determine the center of each bin) the optimrd bin radius is /~Limes larger, The angular resolution of the detector is 0.7' and I%", ZP * 0.02 therefore a circular bin with radius 2.1°is used for this search.The search window that maximises the sensitivity to evaporating black holes depends on the energy threshold of the detector and the observed cosmic-ray background rate.
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