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Novel Method for Incorporating Model Uncertainties into Gravitational Wave Parameter Estimates
Christopher J. Moore, Jonathan R. Gair
Posterior distributions on parameters computed from experimental data using Bayesian techniques are only as accurate as the models used to construct them. In many applications thes…
The sensitivity of pulsar timing arrays
Christopher J. Moore
Simple analytic expressions are derived for the sensitivity curve of a pulsar timing array (PTA) to both a monochromatic source of gravitational waves and an isotropic stochastic b…
Gravitational-wave sensitivity curves
Christopher J. Moore, Robert H. Cole, Christopher P. L. Berry
There are several common conventions in use by the gravitational-wave community to describe the amplitude of sources and the sensitivity of detectors. These are frequently confused…
Estimating the sensitivity of pulsar timing arrays
Christopher J. Moore, Stephen R. Taylor, Jonathan R. Gair
The sensitivity curve of a canonical pulsar timing array is calculated for two types of source: a monochromatic wave and a stochastic background. These calculations are performed i…