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Magnetar vibrational modes are theorized to be associated with energeticX-ray flares. Regular searches for gravitational waves from these modes havebeen performed by Advanced LIGO and Advanced Virgo, with no detections so far.Presently, search results are given in limits on the root-sum-square of theintegrated gravitational-wave strain. However, the increased sensitivity ofcurrent detectors and the promise of future detectors invite the considerationof more astrophysically motivated methods. We present a framework foraugmenting gravitational wave searches to measure or place direct limits onmagnetar astrophysical properties in various search scenarios using a set ofphenomenological and analytic models.

Prospects for Neutron Star Parameter Estimation using Gravitational Waves from f-modes Associated with Magnetar Flares