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All-sky searches for gravitational-wave pulsars are generally limited insensitivity by the finite availability of computing resources. Semicoherentsearches are a common method of maximizing search sensitivity given a fixedcomputing budget. The work of Wette and Prix [Phys. Rev. D 88, 123005 (2013)]and Wette [Phys. Rev. D 92, 082003 (2015)] developed a semicoherent searchmethod which uses metrics to construct the banks of pulsar signal templatesneeded to search the parameter space of interest. In this work we extend therange of validity of the parameter-space metrics using an empirically-derivedrelationship between the resolution (or mismatch) of the template banks and themismatch of the overall search. This work has important consequences for theoptimization of metric-based semicoherent searches at fixed computing cost.

Empirically extending the range of validity of parameter-space metrics for all-sky searches for gravitational-wave pulsars