activity
20152017
most citedEccentric, nonspinning, inspiral, Gaussian-process merger approximant for the detection and characterization of eccentric binary black hole mergers

156 citations · 302 across the 5 of their papers we have counts for

collaborators

7 papers

gr-qc2017156 cited

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…

gr-qc201750 cited

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…

gr-qc201732 cited

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…

gr-qc201664 cited

Black hole kicks as new gravitational wave observables

Davide Gerosa, Christopher J. Moore

Generic black hole binaries radiate gravitational waves anisotropically, imparting a recoil, or kick, velocity to the merger remnant. If a component of the kick along the line of s…

stat.ML2016

Fast methods for training Gaussian processes on large data sets

Christopher J. Moore, Alvin J. K. Chua, Christopher P. L. Berry +1

Gaussian process regression (GPR) is a non-parametric Bayesian technique for interpolating or fitting data. The main barrier to further uptake of this powerful tool rests in the co…

gr-qc2015

Testing the "no-hair" property of black holes with X-ray observations of accretion disks

Christopher J. Moore, Jonathan R. Gair

Accretion disks around black holes radiate a significant fraction of the rest mass of the accreting material in the form of thermal radiation from within a few gravitational radii…