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Free keywords:
Astrophysics, Instrumentation and Methods for Astrophysics, astro-ph.IM, Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE,General Relativity and Quantum Cosmology, gr-qc
Abstract:
A number of open problems hinder our present ability to extract scientific
information from data that will be gathered by the near-future
gravitational-wave mission LISA. Many of these relate to the modeling,
detection and characterization of signals from binary inspirals with an extreme
$(\lesssim10^{-4})$ component-mass ratio. In this paper, we draw attention to
the issue of systematic error in parameter estimation due to the use of fast
but approximate waveform models; this is found to be relevant for
extreme-mass-ratio inspirals even in the case of waveforms with $\gtrsim90\%$
overlap accuracy and moderate ($\gtrsim30$) signal-to-noise ratios. A scheme
that uses Gaussian processes to interpolate and marginalize over waveform error
is adapted and investigated as a possible precursor solution to this problem.
Several new methodological results are obtained, and the viability of the
technique is successfully demonstrated on a three-parameter example in the
setting of the LISA Data Challenge.
