748 citations · 3.7k across the 47 of their papers we have counts for
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Eccentric, nonspinning, inspiral, Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers
E. A. Huerta, C. J. Moore, Prayush Kumar +10
We present , a time domain, inspiral-merger-ringdown waveform model that describes non-spinning binary black holes systems that evolve on moderately eccentric orbi…
Long-lived inverse chirp signals from core collapse in massive scalar-tensor gravity
Ulrich Sperhake, Christopher J. Moore, Roxana Rosca +3
This letter considers stellar core collapse in massive scalar--tensor theories of gravity. The presence of a mass term for the scalar field allows for dramatic increases in the rad…
An astrometric search method for individually resolvable gravitational wave sources with Gaia
Christopher J. Moore, Deyan P. Mihaylov, Anthony Lasenby +1
Gravitational waves (GWs) cause the apparent position of distant stars to oscillate with a characteristic pattern on the sky. Astrometric measurements (e.g. those made by Gaia) the…
Gravitational waves from extreme mass ratio inspirals around bumpy black holes
Christopher J. Moore, Alvin J. K. Chua, Jonathan R. Gair
The space based interferometer LISA will be capable of detecting the gravitational waves emitted by stellar mass black holes or neutron stars slowly inspiralling into the supermass…
The Fast and the Fiducial: Augmented kludge waveforms for detecting extreme-mass-ratio inspirals
Alvin J. K. Chua, Christopher J. Moore, Jonathan R. Gair
The extreme-mass-ratio inspirals (EMRIs) of stellar-mass compact objects into massive black holes are an important class of source for the future space-based gravitational-wave det…