activity
19962022
most citedGravitational wave extraction from an inspiraling configuration of merging black holes

1.3k citations · 6.1k across the 59 of their papers we have counts for

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42 papers · 1 filter

gr-qc2022★ 7 cited

Fully data-driven time-delay interferometry with time-varying delays

Quentin Baghi, John G. Baker, Jacob Slutsky +1

Raw space-based gravitational-wave data like LISA's phase measurements are dominated by laser frequency noise. The standard technique to make this data usable for science is time-d…

gr-qc2020★ 140 cited

Exploring the Bayesian parameter estimation of binary black holes with LISA

Sylvain Marsat, John G. Baker, Tito Dal Canton

The space-based gravitational wave detector LISA will observe mergers of massive black hole binary systems (MBHBs) to cosmological distances, as well as inspiralling stellar-origin…

gr-qc2018★ 6 cited

Fourier-domain modulations and delays of gravitational-wave signals

Sylvain Marsat, John G. Baker

We present a Fourier-domain approach to modulations and delays of gravitational wave signals, a problem which arises in two different contexts. For space-based detectors like LISA,…

gr-qc2013★ 51 cited

The Transient Gravitational-Wave Sky

Nils Andersson, John Baker, Kris Belczynski +44

Interferometric detectors will very soon give us an unprecedented view of the gravitational-wave sky, and in particular of the explosive and transient Universe. Now is the time to…

gr-qc2012★ 310 cited

Testing General Relativity with Low-Frequency, Space-Based Gravitational-Wave Detectors

Jonathan R. Gair, Michele Vallisneri, Shane L. Larson +1

We review the tests of general relativity that will become possible with space-based gravitational-wave detectors operating in the ~0.01mHz - 1Hz low-frequency band. The fundamenta…

gr-qc2012★ 66 cited

Decoding mode-mixing in black-hole merger ringdown

Bernard J. Kelly, John G. Baker

Optimal extraction of information from gravitational-wave observations of binary black-hole coalescences requires detailed knowledge of the waveforms. Current approaches for repres…

gr-qc2012★ 63 cited

Systematic biases in parameter estimation of binary black-hole mergers

Tyson B. Littenberg, John G. Baker, Alessandra Buonanno +1

Parameter estimation of binary-black-hole merger events in gravitational-wave data relies on matched-filtering techniques, which, in turn, depend on accurate model waveforms. Here…

gr-qc2012★ 21 cited

Comparison of Atom Interferometers and Light Interferometers as Space-Based Gravitational Wave Detectors

John G. Baker, James Ira Thorpe

We consider a class of proposed gravitational wave detectors based on multiple atomic interferometers separated by large baselines and referenced by common laser systems. We comput…

gr-qc2011★ 33 cited

Mergers of black-hole binaries with aligned spins: Waveform characteristics

Bernard J. Kelly, John G. Baker, William D. Boggs +2

We conduct a descriptive analysis of the multipolar structure of gravitational-radiation waveforms from equal-mass aligned-spin mergers, following an approach first presented in th…

gr-qc2011★ 30 cited

Sky localization of complete inspiral-merger-ringdown signals for nonspinning massive black hole binaries

Sean T. McWilliams, Ryan N. Lang, John G. Baker +1

We investigate the capability of LISA to measure the sky position of equal-mass, nonspinning black hole binaries, combining for the first time the entire inspiral-merger-ringdown s…

gr-qc2010★ 247 cited

Black-hole binaries, gravitational waves, and numerical relativity

Joan M. Centrella, John G. Baker, Bernard J. Kelly +1

Understanding the predictions of general relativity for the dynamical interactions of two black holes has been a long-standing unsolved problem in theoretical physics. Black-hole m…

gr-qc2010★ 23 cited

The Final Merger of Black-Hole Binaries

Joan M. Centrella, John G. Baker, Bernard J. Kelly +1

Recent breakthroughs in the field of numerical relativity have led to dramatic progress in understanding the predictions of General Relativity for the dynamical interactions of two…

gr-qc2010★ 32 cited

Improved Time-Domain Accuracy Standards for Model Gravitational Waveforms

Lee Lindblom, John G. Baker, Benjamin J. Owen

Model gravitational waveforms must be accurate enough to be useful for detection of signals and measurement of their parameters, so appropriate accuracy standards are needed. Yet t…

gr-qc2010★ 74 cited

Observing mergers of non-spinning black-hole binaries

Sean T. McWilliams, Bernard J. Kelly, John G. Baker

Advances in the field of numerical relativity now make it possible to calculate the final, most powerful merger phase of binary black-hole coalescence for generic binaries. The sta…

gr-qc2009★ 33 cited

Impact of mergers on LISA parameter estimation for nonspinning black hole binaries

Sean T. McWilliams, James Ira Thorpe, John G. Baker +1

We investigate the precision with which the parameters describing the characteristics and location of nonspinning black hole binaries can be measured with the Laser Interferometer…

gr-qc2009★ 55 cited

Status of NINJA: the Numerical INJection Analysis project

Benjamin Aylott, John G. Baker, William D. Boggs +74

The 2008 NRDA conference introduced the Numerical INJection Analysis project (NINJA), a new collaborative effort between the numerical relativity community and the data analysis co…

gr-qc2009★ 140 cited

Testing gravitational-wave searches with numerical relativity waveforms: Results from the first Numerical INJection Analysis (NINJA) project

Benjamin Aylott, John G. Baker, William D. Boggs +74

The Numerical INJection Analysis (NINJA) project is a collaborative effort between members of the numerical relativity and gravitational-wave data analysis communities. The purpose…

gr-qc2009★ 82 cited

The Samurai Project: verifying the consistency of black-hole-binary waveforms for gravitational-wave detection

Mark Hannam, Sascha Husa, John G. Baker +16

We quantify the consistency of numerical-relativity black-hole-binary waveforms for use in gravitational-wave (GW) searches with current and planned ground-based detectors. We comp…

gr-qc2008★ 100 cited

The Mock LISA Data Challenges: from Challenge 1B to Challenge 3

Stanislav Babak, John G. Baker, Matthew J. Benacquista +27

The Mock LISA Data Challenges are a programme to demonstrate and encourage the development of LISA data-analysis capabilities, tools and techniques. At the time of this workshop, t…

gr-qc2008★ 129 cited

Mergers of nonspinning black-hole binaries: Gravitational radiation characteristics

John G. Baker, William D. Boggs, Joan Centrella +3

We present a detailed descriptive analysis of the gravitational radiation from black-hole binary mergers of nonspinning black holes, based on numerical simulations of systems varyi…

gr-qc2007★ 64 cited

Report on the second Mock LISA Data Challenge

Stanislav Babak, John G. Baker, Matthew J. Benacquista +40

The Mock LISA Data Challenges are a program to demonstrate LISA data-analysis capabilities and to encourage their development. Each round of challenges consists of several data set…

gr-qc2007★ 144 cited

Anatomy of the binary black hole recoil: A multipolar analysis

Jeremy D. Schnittman, Alessandra Buonanno, James R. van Meter +5

We present a multipolar analysis of the gravitational recoil computed in recent numerical simulations of binary black hole (BH) coalescence, for both unequal masses and non-zero, n…

gr-qc2007★ 286 cited

Toward faithful templates for non-spinning binary black holes using the effective-one-body approach

Alessandra Buonanno, Yi Pan, John G. Baker +4

We present an accurate approximation of the full gravitational radiation waveforms generated in the merger of non-eccentric systems of two non-spinning black holes. Utilizing infor…

gr-qc2007★ 176 cited

A data-analysis driven comparison of analytic and numerical coalescing binary waveforms: nonspinning case

Yi Pan, Alessandra Buonanno, John G. Baker +5

We compare waveforms obtained by numerically evolving nonspinning binary black holes to post-Newtonian (PN) template families currently used in the search for gravitational waves b…