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How Many Templates for GW Chirp Detection? The Minimal-Match Issue Revisited

R. P. Croce·Th. Demma·M. Longo·S. Marano·V. Matta·V. Pierro·I. M. Pinto
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Abstract

In a recent paper dealing with maximum likelihood detection of gravitational wave chirps from coalescing binaries with unknown parameters we introduced an accurate representation of the no-signal cumulative distribution of the supremum of the whole correlator bank. This result can be used to derive a refined estimate of the number of templates yielding the best tradeoff between detector's performance (in terms of lost signals among those potentially detectable) and computational burden.

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R. P. Croce, Th. Demma, M. Longo, S. Marano, V. Matta, V. Pierro, I. M. Pinto. 2004-04-24. How Many Templates for GW Chirp Detection? The Minimal-Match Issue Revisited. https://doi.org/10.1088/0264-9381%2F21%2F21%2F013

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